Difference between revisions of "List of accreting X-ray pulsars"

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(Updated citations for sources without Gaia distances)
(Moved Gaia distances back to separate table.)
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= List of accreting X-ray pulsars =
 
= List of accreting X-ray pulsars =
−
{| class="wikitable"
+
{| class="wikitable sortable"
 
! Source
 
! Source
 
! RA
 
! RA
 
! Dec
 
! Dec
−
! Distance (kpc)
+
! l
 +
! b
 
! Pspin (s)
 
! Pspin (s)
 
! Porbit (d)
 
! Porbit (d)
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! Notes
 
! Notes
 
|-
 
|-
−
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 62<ref name="graczyk14">Distance to SMC. See Graczyk, D. et al., ApJ 780, 59 ([https://ui.adsabs.harvard.edu/#abs/2014ApJ...780...59G/abstract NASA ADS])</ref> || 292 || || [[List of Be X-ray Binaries|BeXRB]]? ||  || T || aka SXP 292
+
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 ||   || [[List of Be X-ray Binaries|BeXRB]]? ||  || T || aka SXP 292
 
|-
 
|-
  
−
| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 62<ref name="graczyk14" /> || 2.76 || 82|| [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
+
| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
 
|-
 
|-
  
−
| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 12.3 (+2.0, -1.7)<ref name="bailerjones18">Bailer-Jones, C.A.L. et al., submitted to ApJ as of 11 July 2018 ([https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract NASA ADS])</ref> || 175 || || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
+
| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 ||   || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
 
|-
 
|-
  
−
| [[SMC X-1]] || 19.271456 || -73.443343 || 62<ref name="graczyk14" /> || 0.71 || 3.892 || SG ||  || P || eclipsing
+
| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG ||  || P || eclipsing
 
|-
 
|-
  
−
| [[3A 0114+650]] || 19.511228 || 65.291623 || 7.2 <ref name="reig96">Reig, P. et al., 1996, ApJ 311, 879 ([https://ui.adsabs.harvard.edu/#abs/1996A&A...311..879R NASA ADS])</ref> || 9828 || 11.6 || SG ||  || P || 30.7 d superorbital modulation
+
| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG ||  || P || 30.7 d superorbital modulation
 
|-
 
|-
  
−
| [[4U 0115+634]] || 19.633194 || 63.742522 || 7.2 (+1.5, -1.1) || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
+
| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
 
|-
 
|-
  
−
| [[SXP 265]] || 23.214439 || -74.429258 || 62<ref name="graczyk14" /> || 264.52 || || [[List of Be X-ray Binaries|BeXRB]] ||  || PT || SMC region, persistent low luminosity, one type I outburst
+
| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] ||  || PT || SMC region, persistent low luminosity, one type I outburst
 
|-
 
|-
  
−
| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 2.50 (+0.22, -0.19) || 1412 || 330 || [[List of Be X-ray Binaries|BeXRB]] ||  || T || a.k.a. V* V831 Cas
+
| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] ||  || T || aka V* V831 Cas
 
|-
 
|-
  
−
| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 7.4 (+1.1, -0.9) || 469 || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
+
| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? ||   || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
 
|-
 
|-
  
−
| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 6.9 (+1.6, -1.2) || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
+
| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] ||   || T || Galactic ULX?
 
|-
 
|-
  
−
| [[V 0332+53]] || 53.749630 || 53.173140 || 5.1 (+1.1, -0.8) || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
+
| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
 
|-
 
|-
  
−
| [[X Per]] || 58.846151 || 31.045836 || 0.79 +/- 0.04 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || || P || magnetar?
+
| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
 
|-
 
|-
  
−
| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 3.2 (+0.7, -0.5) || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] ||  || P || a.k.a. LS V+44 17, persistent, but with outbursts
+
| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] ||  || P || aka LS V+44 17, persistent, but with outbursts
 
|-
 
|-
  
−
| [[LXP 169]] || 76.981153 || -68.418135 || 50<ref name="pietrzynski13">Distance to LMC. See Pietrzynski, G. et al., 2013, Nature 495, 76 ([https://ui.adsabs.harvard.edu/#abs/2013Natur.495...76P])</ref> || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] ||  || T? || NS eclipsing companion, LMC source
+
| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] ||  || T? || NS eclipsing companion
 
|-
 
|-
  
−
| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 50<ref name="pietrzynski13" /> || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] ||  || T? ||  LMC source
+
| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 ||   || [[List of Be X-ray Binaries|BeXRB]] ||  || T? ||   
 
|-
 
|-
  
−
| [[LMC X-4]] || 83.206501 || -66.370332 || 50<ref name="pietrzynski13" /> || 13.5 || 1.4 || SG ||  || P || superorbital variation ~30 d
+
| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG ||  || P || superorbital variation ~30 d
 
|-
 
|-
  
−
| [[1A 0535+26]] || 84.727393 || 26.315776 || 2.13 (+0.26, -0.21) || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||  
+
| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
 
|-
 
|-
  
−
| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 1.6 (+2.2, -0.8) || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] ||  || T || low luminosity
+
| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 ||   || [[List of Be X-ray Binaries|BeXRB]] ||  || T || low luminosity
 
|-
 
|-
  
−
| [[MXB 0656-07]] || 104.572030 || -7.209774 || 5.1 (+1.4, -1.0) || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] ||  || a.k.a XTE J0658-073
+
| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] ||  || aka XTE J0658-073
 
|-
 
|-
  
−
| [[3A 0726-260]] || 112.223241 || -26.108019 || 9.5 (+3.1, -2.2) || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
+
| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
 
|-
 
|-
  
−
| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 6.8 (+1.2, -1.0) || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
+
| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
 
|-
 
|-
  
−
| [[GS 0834-430]] || 128.981072 || -43.185598 || 5.5 (+2.5, -1.7) || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
+
| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
 
|-
 
|-
  
−
| [[Vela X-1]] || 135.528560 || -40.554654 || 2.42 (+0.19, -0.17) || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
+
| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
 
|-
 
|-
  
−
| [[GRO J1008-57]] || 152.439620 || -58.292035 || 5.8<ref name="riquelme12">Riquelme, M., Torrejon, J.M., and Negueruela, I., 2012, A&A 539, 114 ([https://ui.adsabs.harvard.edu/#abs/2012A&A...539A.114R/abstract NASA ADS]</ref>  || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
+
| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
 
|-
 
|-
  
−
| [[4U 1036-56]] || 159.397094 || -56.798840 || 5.0 (+1.1, -0.8) || 862 || || [[List of Be X-ray Binaries|BeXRB]] ||  || P? || a.k.a. RX J1037.5-564/LS 1698
+
| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 ||   || [[List of Be X-ray Binaries|BeXRB]] ||  || P? || aka RX J1037.5-564/LS 1698
 
|-
 
|-
  
−
| [[1A 1118-616]] || 170.238174 || -61.916707 || 2.93 (+0.26, -0.22) || 407 || 24 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||   
+
| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||   
 
|-
 
|-
  
−
| [[Cen X-3]] || 170.312856 || -60.623776 || 6.4 (+1.4, -1.1) || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
+
| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
 
|-
 
|-
  
−
| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 9.1 (+2.2, -1.6) || 297 || 14.4 || SG ||  ||  || (V* V830 Cen) varying luminosity states
+
| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG ||  ||  || (V* V830 Cen) varying luminosity states
 
|-
 
|-
  
−
| [[4U 1145-619]] || 177.000032 || -62.206910 || 2.23 (+0.20, -0.17) || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] ||  || PT ||   
+
| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] ||  || PT ||   
 
|-
 
|-
  
−
| [[GX 301-2]] || 186.656453 || -62.770359 || 3.5 (+0.6, -0.5) || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
+
| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
 
|-
 
|-
  
−
| [[3A 1239-599]] || 190.508997 || -60.200951 || 2.9 (+2.4, -1.3) || 191 || ||  ||  ||  ||   
+
| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 ||   ||  ||  ||  ||   
 
|-
 
|-
  
−
| [[GX 304-1]] || 195.321198 || -61.601845 || 2.01 (+0.15, -0.13) || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
+
| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
 
|-
 
|-
  
−
| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 3.5 (+2.6, -1.7) || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? ||  ||  ||   
+
| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? ||  ||  ||   
 
|-
 
|-
  
−
| [[2S 1417-624]] || 215.303896 || -62.698168 || 3.8 (+2.8, -1.8) || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
+
| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
 
|-
 
|-
  
−
| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 3.0 (+2.6, -1.5) || 437 || || [[List of Be X-ray Binaries|BeXRB]]? ||  ||  ||   
+
| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 ||   || [[List of Be X-ray Binaries|BeXRB]]? ||  ||  ||   
 
|-
 
|-
  
−
| [[4U 1538-52]] || 235.597300 || -52.386011 || 6.6 (+2.2, -1.5) || 526 || 3.72 || SG || [[List of cyclotron line sources|C]] || P ||   
+
| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||   
 
|-
 
|-
  
−
| [[2S 1553-542]] || 239.452345 || -54.416113 || 3.5 (+2.6, -1.5) || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? ||  || P || Occasional outbursts
+
| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? ||  || P || Occasional outbursts
 
|-
 
|-
  
−
| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 2.3 (+0.8, -0.5) || || || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  ||   
+
| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 ||   ||   || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  ||   
 
|-
 
|-
  
−
| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 9.8 (+3.2, -2.4) || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
+
| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
 
|-
 
|-
  
−
| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 5.2 (+2.8, -1.9) || || || SG ||  || P || super absorbed source
+
| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 ||   ||   || SG ||  || P || super absorbed source
 
|-
 
|-
  
−
| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 1.3 (+0.6, -0.4) || 1309 || 8.986 || SG ||  || P || aka 2FGL J1632.4-4753c
+
| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG ||  || P || aka 2FGL J1632.4-4753c
 
|-
 
|-
  
−
| [[4U 1626-67]] || 248.069509 || -67.461207 || 3.5 (+2.3, -1.3) || 7.7 || 0.029 || WD? || [[List of cyclotron line sources|C]] ||   || Torque reversals. Only UCXB with a CRSF.
+
| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
 
|-
 
|-
  
−
| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 5-6 or 12-13 <ref name="lutovinov05">Lutovinov, A., Revnivtsev, M., Gilfanov, M., et al. 2005, A&A, 444 ([https://ui.adsabs.harvard.edu/#abs/2005A&A...444..821L/abstract NASA ADS])</ref> || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  || Distances estimates depend on which part of the Norma arm the source is assumed to reside in.
+
| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 ||   || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  ||
 
|-
 
|-
  
−
| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 4.0 (+2.7, -1.7) || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  || a.k.a. AX J1639.0-4642
+
| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  || aka AX J1639.0-4642
 
|-
 
|-
  
−
| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 2.7 (+0.5, -0.4) || 228 || 30.243 ||  ||  || P || aka 2MASS J16463526-4507045
+
| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 ||  ||  || P || aka 2MASS J16463526-4507045
 
|-
 
|-
  
−
| [[Her X-1]] || 254.457539 || 35.342324 || 5.0 (+0.8, -0.6) || 1.24 || 1.7 || IMXB || [[List of cyclotron line sources|C]] || P ||   
+
| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||   
 
|-
 
|-
  
−
| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 3.4 (+2.6, -1.5) || 715 || || [[List of Be X-ray Binaries|BeXRB]]? ||  ||  ||   
+
| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 ||   || [[List of Be X-ray Binaries|BeXRB]]? ||  ||  ||   
 
|-
 
|-
  
−
| [[OAO 1657-415]] || 255.202665 || -41.654882 || 2.2 (+0.7, -0.5) || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
+
| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
 
|-
 
|-
  
−
| [[4U 1700-37]] || 255.986566 || -37.844121 || 1.75 (+0.24, -0.19) || || 3.4 || SG || || P || No pulsations, eclipsing source
+
| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 ||   || 3.4 || SG ||   || P || No pulsations; eclipsing source
 
|-
 
|-
  
−
| [[4U 1700+24]] || 256.643762 || 23.971820 || 0.536 +/- 0.010 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  ||   
+
| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 ||   || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  ||   
 
|-
 
|-
  
−
| [[EXO 1722-363]] || 261.296681 || -36.284621 || 4.0 (+2.3, -1.3) || || 9.74 || HMXB ||  ||  || a.k.a. IGR J17252–3616, heavily absorbed, eclipsing
+
| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB ||  ||  || aka IGR J17252–3616, heavily absorbed, eclipsing
 
|-
 
|-
  
−
| [[GX 1+4]] || 263.008955 || -24.745600 || 7.6 (+4.3, -2.8) || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] ||  || P || Pulse period evolving rapidly
+
| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] ||  || P || Pspin evolving rapidly
 
|-
 
|-
  
−
| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 1.4 (+1.6, -0.5) || 626 || || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  || a. k.a. AX_J1740.2-2903
+
| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 ||   || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  || a. k.a. AX_J1740.2-2903
 
|-
 
|-
  
−
| [[GRO J1744-28]] || 266.139419 || -28.744480 || 1.3 (+1.2, -0.5) || 0.47 || 11.8 || LMXB ||  || T || "Bursting Pulsar"
+
| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB ||  || T || "Bursting Pulsar"
 
|-
 
|-
  
−
| [[GRO J1750-27]] || 267.291434 || -26.639700 || 18<ref name="scott97">Scott, D.M., et al., 1997, ApJ 488, 831 ([https://ui.adsabs.harvard.edu/#abs/1997ApJ...488..831S/abstract NASA ADS])</ref>|| 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? ||  || P || a.k.a. AX J1749.1-2639
+
| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? ||  || P || aka AX J1749.1-2639
 
|-
 
|-
  
−
| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 2.7 (+0.5, -0.4) || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||  
+
| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 ||   || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
 
|-
 
|-
  
−
| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 1.5 (+2.8, -0.7) || 139.6 || 4.57 || SG ||  || P || a.k.a. IGR J18027-2016
+
| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG ||  || P || aka IGR J18027-2016
 
|-
 
|-
  
−
| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 10<ref name="nucita07">Nucita, A.A., Carpano, S., and Guainazzi, M., 2007, A&A 474, L1 ([<https://ui.adsabs.harvard.edu/#abs/2007A%26A...474L...1N/abstract NASA ADS])</ref> || 494 || || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  || Likely a magnetic CV, not a SyXB, according to Masetti et al. (2012)<ref name="masetti12">Masetti, N., Nucita, A.A., and Parisi, P., 2012, A&A 544, 114 ([https://ui.adsabs.harvard.edu/#abs/2012A&A...544A.114M/abstract NASA ADS])</ref>
+
| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 ||   || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  ||
 
|-
 
|-
  
−
| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 5.1 (+4.3, -2.6) || 0.0025 || 0.837 || LMXB ||  ||  || a.k.a. V* V4580 Sgr, disk accretor(?)
+
| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB ||  ||  || aka V* V4580 Sgr, disk accretor(?)
 
|-
 
|-
  
−
| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 1.4 (+2.5, -0.7) || 142.9 || 151 || [[List of Be X-ray Binaries|BeXRB]]? ||  || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
+
| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? ||  || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
 
|-
 
|-
  
−
| [[IGR J18179-1621]] || 274.467048 || -16.359400 || || 11.82 || ||  || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
+
| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 ||   ||  || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
 
|-
 
|-
  
−
| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 3.5-6<ref name="segreto13">Segreto, A. et al., 2013, A&A 558, 99 ([https://ui.adsabs.harvard.edu/#abs/2013A&A...558A..99S/abstract NASA ADS])</ref> || 152 || || HMXB ||  || ? ||  Distance assumes a B0 companion.
+
| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 ||   ||   ||  ||   ||   
 
|-
 
|-
  
−
| [[3A 1822-371]] || 276.445028 || -37.105158 || 6.1 (+2.7, -1.6) || 0.59 || 0.23 || LMXB ||  ||  ||   
+
| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB ||  ||  ||   
 
|-
 
|-
  
−
| [[Sct X-1]] || 278.857602 || -7.614004 || 4-10 <ref name="nebot15">Nebot Gomez-Moran, A., et al., MNRAS 452, 884([https://ui.adsabs.harvard.edu/#abs/2015MNRAS.452..884N/abstract NASA ADS])</ref>|| 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  ||  Distance estimates depend on assumed spectral class of companion.
+
| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  ||   
 
|-
 
|-
  
−
| [[GS 1843+00]] || 281.403474 || 0.863160 || 2.3 (+2.0, -1.0) || || ||  ||  || T ||   
+
| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 ||   ||   ||  ||  || T ||   
 
|-
 
|-
  
−
| [[2S 1845-024]] || 282.075590 || -2.419729 || 10<ref name="finger99">Finger, M., et al., 1999, ApJ 517, 449 ([https://ui.adsabs.harvard.edu/#abs/1999ApJ...517..449F/abstract NASA ADS])</ref> || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? ||  || T || a.k.a. GS 1843-02; distance based on spiral arm location
+
| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? ||  || T || aka GS 1843-02
 
|-
 
|-
  
−
| [[XTE J1855-026]] || 283.876680 || -2.604678 || 8.1 (+2.6, -1.8) || 361 || 6.1 || SG ||  ||  ||   
+
| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG ||  ||  ||   
 
|-
 
|-
  
−
| [[XTE J1858+034]] || 284.678379 || 3.439739 || 1.55 (+0.28, -0.21) || || 221 ||  ||  || T ||   
+
| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 ||   || 221 ||  ||  || T ||   
 
|-
 
|-
  
−
| [[XTE J1859+083]] || 284.778177 || 8.246352 || 2.7 (+2.4, -1.5) || 9.8 || ||  ||  || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
+
| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 ||   ||  ||  || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
 
|-
 
|-
  
−
| [[4U 1901+03]] || 285.903524 || 3.190426 || 2.2 (+2.2, -1.3) || || ||  ||  || T ||   
+
| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 ||   ||   ||  ||  || T ||   
 
|-
 
|-
  
−
| [[XTE J1906+090]] || 286.197769 || 9.044912 || 2.8 (+2.4, -1.4) || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? ||  ||  ||   
+
| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 ||   || [[List of Be X-ray Binaries|BeXRB]]? ||  ||  ||   
 
|-
 
|-
  
−
| [[4U 1907+09]] || 287.408533 || 9.829777 || 4.4 (+2.1, -1.3) || 442 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||   
+
| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||   
 
|-
 
|-
  
−
| [[4U 1909+07]] || 287.700872 || 7.597657 || 2.6 (+2.3, -1.4) || 604 || 4.4 || SG ||  || P ||   
+
| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG ||  || P ||   
 
|-
 
|-
  
−
| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 2.8 (+2.4, -1.4) || || 13.55 || HMXB ||  || ? ||   
+
| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 ||   || 13.55 || HMXB ||  || ? ||   
 
|-
 
|-
  
−
| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 3.0 (+2.5, -1.6) || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
+
| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 ||   || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
 
|-
 
|-
  
−
| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 2.9 (+2.5, -1.5) || 12.5 || 116 || [[List of Be X-ray Binaries|BeXRB]]? ||  || T ||   
+
| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? ||  || T ||   
 
|-
 
|-
  
−
| [[XTE J1946+274]] || 296.413975 || 27.365400 || 12.6 (+3.9, -2.9) || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||   
+
| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||   
 
|-
 
|-
  
−
| [[KS 1947+300]] || 297.397839 || 30.208809 || 15.2 (+3.7, -2.8) || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||   
+
| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||   
 
|-
 
|-
  
−
| [[3A 1954+319]] || 298.926399 || 32.096931 || 3.3 (+1.0, -0.7) || 19100 || || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  ||   
+
| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 ||   || [[List of symbiotic X-ray binaries|SyXB]] ||  ||  ||   
 
|-
 
|-
  
−
| [[EXO 2030+375]] || 308.063627 || 37.637433 || 3.6 (+1.4, -0.9) || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] ||  || T || regular outbursts
+
| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] ||  || T || regular outbursts
 
|-
 
|-
  
−
| [[GRO J2058+42]] || 314.698059 || 41.776980 || 8.0 (+1.2, -1.0) || || ||  ||  || T ||   
+
| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 ||   ||   ||  ||  || T ||   
 
|-
 
|-
  
−
| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 6.4 (+0.9, -0.7) || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
+
| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
 
|-
 
|-
  
−
| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 7.8 (+1.4, -1.1) || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] ||  || P? || Varying levels of activity
+
| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] ||  || P? || Varying levels of activity
 
|-
 
|-
  
−
| [[Cep X-4]] || 324.877853 || 56.986219 || 10.2 (+2.2, -1.6) || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||   
+
| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||   
 
|-
 
|-
  
−
| [[4U 2206+54]] || 331.984289 || 54.518433 || 3.3 +/- 0.4 || 5560 || 19.25 || SG ||  || P || magnetar?
+
| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG ||  || P || magnetar?
 
|-
 
|-
  
−
| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 8.0 (+1.4, -1.1) || 1247 || 262 || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
+
| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] ||  || T ||   
 
|-
 
|-
  
−
| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 8.1 (+2.3, -1.6) || 46.7 || || Be? ||  || P? ||   
+
| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 ||   || [[List of Be X-ray Binaries|BeXRB]]? ||  || P? ||   
 
|-
 
|-
 
|}
 
|}
−
 
−
All distances with uncertainties are from Gaia data release 2, as described by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Note that these should be taken with a grain of salt and are dependent on the priors selected by Bailer-Jones et al. - as an example, the Magellanic cloud sources show up in Gaia DR2 as having distances of ~7 kpc, when they are actually 45 or 60 kpc away.
 
−
 
−
 
  
 
= Location in the Galaxy =
 
= Location in the Galaxy =
Line 618: Line 615:
 
|-
 
|-
 
|}
 
|}
 +
 +
The following table describes parallax distances as computed by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Note that these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al. - as an example, the Magellanic cloud sources show up in Gaia DR2 as having distances of ~7 kpc, when they are actually 45 or 60 kpc away.
 +
 +
{| class="wikitable"
 +
! Source
 +
! Gaia distance
 +
|-
 +
| [[RX J0101.8-7223]] || 12.3 (+2.0, -1.7)
 +
|-
 +
 +
| [[3A 0114+650]] || 6.6 (+1.6, -1.2)
 +
|-
 +
 +
| [[4U 0115+634]] || 7.2 (+1.5, -1.1)
 +
|-
 +
 +
| [[RX J0146.9+6121]] || 2.50 (+0.22, -0.19)
 +
|-
 +
 +
| [[IGR J01583+6713]] || 7.4 (+1.1, -0.9)
 +
|-
 +
 +
| [[Swift J0243.6+6124]] || 6.9 (+1.6, -1.2)
 +
|-
 +
 +
| [[V 0332+53]] || 5.1 (+1.1, -0.8)
 +
|-
 +
 +
| [[X Per]] || 0.79 +/- 0.04
 +
|-
 +
 +
| [[RX J0440.9+4431]] || 3.2 (+0.7, -0.5)
 +
|-
 +
 +
| [[1A 0535+26]] || 2.13 (+0.26, -0.21)
 +
|-
 +
 +
| [[SAX J0635.2+0533]] || 1.6 (+2.2, -0.8)
 +
|-
 +
 +
| [[MXB 0656-07]] || 5.1 (+1.4, -1.0)
 +
|-
 +
 +
| [[3A 0726-260]] || 9.5 (+3.1, -2.2)
 +
|-
 +
 +
| [[RX J0812.4-3114]] || 6.8 (+1.2, -1.0)
 +
|-
 +
 +
| [[GS 0834-430]] || 5.5 (+2.5, -1.7)
 +
|-
 +
 +
| [[Vela X-1]] || 2.42 (+0.19, -0.17)
 +
|-
 +
 +
| [[4U 1036-56]] || 5.0 (+1.1, -0.8)
 +
|-
 +
 +
| [[1A 1118-616]] || 2.93 (+0.26, -0.22)
 +
|-
 +
 +
| [[Cen X-3]] || 6.4 (+1.4, -1.1)
 +
|-
 +
 +
| [[1E1145.1-6141]] || 9.1 (+2.2, -1.6)
 +
|-
 +
 +
| [[4U 1145-619]] || 2.23 (+0.20, -0.17)
 +
|-
 +
 +
| [[GX 301-2]] || 3.5 (+0.6, -0.5)
 +
|-
 +
 +
| [[3A 1239-599]] || 2.9 (+2.4, -1.3)
 +
|-
 +
 +
| [[GX 304-1]] || 2.01 (+0.15, -0.13)
 +
|-
 +
 +
| [[SAX J1324.4-6200]] || 3.5 (+2.6, -1.7)
 +
|-
 +
 +
| [[2S 1417-624]] || 3.8 (+2.8, -1.8)
 +
|-
 +
 +
| [[SAX J1452.8-5949]] || 3.0 (+2.6, -1.5)
 +
|-
 +
 +
| [[4U 1538-522]] || 6.6 (+2.2, -1.5)
 +
|-
 +
 +
| [[2S 1553-542]] || 3.5 (+2.6, -1.5)
 +
|-
 +
 +
| [[IGR J16194-2810]] || 2.3 (+0.8, -0.5)
 +
|-
 +
 +
| [[Swift J1626.6-5156]] || 9.8 (+3.2, -2.4)
 +
|-
 +
 +
| [[IGR J16318-4848]] || 5.2 (+2.8, -1.9)
 +
|-
 +
 +
| [[IGR J16320-4751]] || 1.3 (+0.6, -0.4)
 +
|-
 +
 +
| [[4U 1626-67]] || 3.5 (+2.3, -1.3)
 +
|-
 +
 +
| [[IGR J16393-4643]] || 4.0 (+2.7, -1.7)
 +
|-
 +
 +
| [[IGR J16465-4507]] || 2.7 (+0.5, -0.4)
 +
|-
 +
 +
| [[Her X-1]] || 5.0 (+0.8, -0.6)
 +
|-
 +
 +
| [[AX J1700.1-4157]] || 3.4 (+2.6, -1.5)
 +
|-
 +
 +
| [[OAO 1657-415]] || 2.2 (+0.7, -0.5)
 +
|-
 +
 +
| [[4U 1700-37]] || 1.75 (+0.24, -0.19)
 +
|-
 +
 +
| [[4U 1700+24]] || 0.536 +/- 0.010
 +
|-
 +
 +
| [[EXO 1722-363]] || 4.0 (+2.3, -1.3)
 +
|-
 +
 +
| [[GX 1+4]] || 7.6 (+4.3, -2.8)
 +
|-
 +
 +
| [[2XMM J174016.0-290337]] || 1.4 (+1.6, -0.5)
 +
|-
 +
 +
| [[GRO J1744-28]] || 1.3 (+1.2, -0.5)
 +
|-
 +
 +
| [[IGR J17544-2619]] || 2.7 (+0.5, -0.4)
 +
|-
 +
 +
| [[SAX J1802.7-2017]] || 1.5 (+2.8, -0.7)
 +
|-
 +
 +
| [[SAX J1808.4-3658]] || 5.1 (+4.3, -2.6)
 +
|-
 +
 +
| [[Swift J1816.7-1613]] || 1.4 (+2.5, -0.7)
 +
|-
 +
 +
| [[3A 1822-371]] || 6.1 (+2.7, -1.6)
 +
|-
 +
 +
| [[GS 1843+00]] || 2.3 (+2.0, -1.0)
 +
|-
 +
 +
| [[XTE J1855-026]] || 8.1 (+2.6, -1.8)
 +
|-
 +
 +
| [[XTE J1858+034]] || 1.55 (+0.28, -0.21)
 +
|-
 +
 +
| [[XTE J1859+083]] || 2.7 (+2.4, -1.5)
 +
|-
 +
 +
| [[4U 1901+03]] || 2.2 (+2.2, -1.3)
 +
|-
 +
 +
| [[XTE J1906+090]] || 2.8 (+2.4, -1.4)
 +
|-
 +
 +
| [[4U 1907+09]] || 4.4 (+2.1, -1.3)
 +
|-
 +
 +
| [[4U 1909+07]] || 2.6 (+2.3, -1.4)
 +
|-
 +
 +
| [[IGR J19140+0951]] || 2.8 (+2.4, -1.4)
 +
|-
 +
 +
| [[IGR J19149+1036]] || 3.0 (+2.5, -1.6)
 +
|-
 +
 +
| [[IGR J19294+1816]] || 2.9 (+2.5, -1.5)
 +
|-
 +
 +
| [[XTE J1946+274]] || 12.6 (+3.9, -2.9)
 +
|-
 +
 +
| [[KS 1947+300]] || 15.2 (+3.7, -2.8)
 +
|-
 +
 +
| [[3A 1954+319]] || 3.3 (+1.0, -0.7)
 +
|-
 +
 +
| [[EXO 2030+375]] || 3.6 (+1.4, -0.9)
 +
|-
 +
 +
| [[GRO J2058+42]] || 8.0 (+1.2, -1.0)
 +
|-
 +
 +
| [[SAX J2103.5+4545]] || 6.4 (+0.9, -0.7)
 +
|-
 +
 +
| [[IGR J21343+4738]] || 7.8 (+1.4, -1.1)
 +
|-
 +
 +
| [[Cep X-4]] || 10.2 (+2.2, -1.6)
 +
|-
 +
 +
| [[4U 2206+54]] || 3.3 +/- 0.4
 +
|-
 +
 +
| [[SAX J2239.3+6116]] || 8.0 (+1.4, -1.1)
 +
|-
 +
 +
| [[IGR J22534+6243]] || 8.1 (+2.3, -1.6)
 +
|-
 +
|}
 +
  
 
= Correlation between luminosity and CRSF energy =
 
= Correlation between luminosity and CRSF energy =

Revision as of 21:06, 12 July 2018


List of accreting X-ray pulsars

Source RA Dec l b Pspin (s) Porbit (d) Type CRSF? Persistent? Notes
CXOU J005047.9-731817 12.699963 -73.305018 302.995436 -43.823153 292 BeXRB? T aka SXP 292
RX J0059.2-7138 14.803112 -71.645828 302.059336 -45.469247 2.76 82? BeXRB? C? T aka SXP 2.76
RX J0101.8-7223 15.467910 -72.392796 301.821935 -44.712961 175 BeXRB T
SMC X-1 19.271456 -73.443343 300.414946 -43.559342 0.71 3.892 SG P eclipsing
3A 0114+650 19.511228 65.291623 125.709976 2.563488 9828 11.6 SG P 30.7 d superorbital modulation
4U 0115+634 19.633194 63.742522 125.923515 1.028265 3.6 24.3 BeXRB C T 5 or more lines
SXP 265 23.214439 -74.429258 299.185905 -42.396387 264.52 ~146 BeXRB PT SMC region, persistent low luminosity, one type I outburst
RX J0146.9+6121 26.750876 61.356573 129.541104 -0.800112 1412 330? BeXRB T aka V* V831 Cas
IGR J01583+6713 29.577033 67.223185 129.352236 5.188723 469? BeXRB C? T controversial claim of CRSF features
Swift J0243.6+6124 40.918432 61.434378 135.934157 1.428788 9.86 27.587 BeXRB T Galactic ULX?
V 0332+53 53.749630 53.173140 146.052090 -2.194026 4.37 34.25 BeXRB C T multiple lines
X Per 58.846151 31.045836 163.081353 -17.136203 830 250.3 BeXRB C? P magnetar?
RX J0440.9+4431 70.247207 44.530344 159.847095 -1.270023 203 155 BeXRB P aka LS V+44 17, persistent, but with outbursts
LXP 169 76.981153 -68.418135 279.245167 -34.534204 168.8 24.3 BeXRB T? NS eclipsing companion
Swift J053041.9-665426 82.675788 -66.907566 276.997292 -32.675902 28.78 BeXRB T?
LMC X-4 83.206501 -66.370332 276.334942 -32.529084 13.5 1.4 SG P superorbital variation ~30 d
1A 0535+26 84.727393 26.315776 181.445049 -2.643537 103 111.1 BeXRB C T
SAX J0635.2+0533 98.822528 5.553870 206.149196 -1.044562 0.0338 BeXRB T low luminosity
MXB 0656-07 104.572030 -7.209774 220.128540 -1.767278 160.4 101.2 BeXRB C aka XTE J0658-073
3A 0726-260 112.223241 -26.108019 240.281581 -4.050430 103.2 34.5 BeXRB T
RX J0812.4-3114 123.118149 -31.247807 249.578200 1.542815 31.9 80 BeXRB T
GS 0834-430 128.981072 -43.185598 262.020238 -1.509977 12.3 105.8 BeXRB T
Vela X-1 135.528560 -40.554654 263.058248 3.929864 283 8.96 SG C P eclipsing
GRO J1008-57 152.439620 -58.292035 282.996761 -1.822544 93.7 249.48 BeXRB C? T outbursts predicted precisely
4U 1036-56 159.397094 -56.798840 285.352684 1.433482 862 BeXRB P? aka RX J1037.5-564/LS 1698
1A 1118-616 170.238174 -61.916707 292.498528 -0.891807 407 24? BeXRB C T
Cen X-3 170.312856 -60.623776 292.090328 0.335524 4.8 2.09 SG C P disk-fed HMXB
1E1145.1-6141 176.868942 -61.953720 295.489729 -0.009704 297 14.4 SG (V* V830 Cen) varying luminosity states
4U 1145-619 177.000032 -62.206910 295.611079 -0.240241 292 187.5 BeXRB PT
GX 301-2 186.656453 -62.770359 300.098061 -0.035212 686 41.5 SG C P very massive companion, strong orbital variability
3A 1239-599 190.508997 -60.200951 301.762822 2.649455 191
GX 304-1 195.321198 -61.601845 304.102702 1.247519 272 132.2 BeXRB C T Strong spectral parameter variations
SAX J1324.4-6200 201.108853 -62.016515 306.792444 0.607646 171 22 BeXRB?
2S 1417-624 215.303896 -62.698168 313.021369 -1.598347 17.6 42.12 BeXRB T
SAX J1452.8-5949 223.207002 -59.820983 317.646019 -0.463151 437 BeXRB?
4U 1538-522 235.597300 -52.386011 327.419660 2.163700 530 3.7 SG C P
2S 1553-542 239.452345 -54.416113 327.942599 -0.857197 9.3 29.56 BeXRB? P Occasional outbursts
IGR J16194-2810 244.888926 -28.127773 349.119337 15.541316 SyXB
Swift J1626.6-5156 246.652146 -51.941848 332.780988 -2.002708 15.4 132.9 BeXRB C T strong flares
IGR J16318-4848 247.951259 -48.816876 335.615970 -0.447754 SG P super absorbed source
IGR J16320-4751 248.009669 -47.874785 336.330340 0.167654 1309 8.986 SG P aka 2FGL J1632.4-4753c
4U 1626-67 248.069509 -67.461207 321.788013 -13.091773 7.67 0.029 UCXB C P Torque reversals; only UCXB with CRSF.
IGR J16358-4726 249.124997 -47.623903 337.023067 -0.213710 5880 SyXB
IGR J16393-4643 249.772382 -46.704006 338.001098 0.075060 912 3.7 SyXB aka AX J1639.0-4642
IGR J16465-4507 251.646902 -45.117960 340.053530 0.135029 228 30.243 P aka 2MASS J16463526-4507045
Her X-1 254.457539 35.342324 58.148987 37.523034 1.24 1.7 IM C P
AX J1700.1-4157 255.018132 -41.968217 344.037996 0.235782 715 BeXRB?
OAO 1657-415 255.202665 -41.654882 344.369539 0.320505 37.7 10.4 SG C? P eclipsing
4U 1700-37 255.986566 -37.844121 347.754446 2.173492 3.4 SG P No pulsations; eclipsing source
4U 1700+24 256.643762 23.971820 45.151698 32.990711 404 SyXB
EXO 1722-363 261.296681 -36.284621 351.495256 -0.354515 ~414 9.74 HMXB aka IGR J17252–3616, heavily absorbed, eclipsing
GX 1+4 263.008955 -24.745600 1.937022 4.794969 170 1161 SyXB P Pspin evolving rapidly
2XMM J174016.0-290337 265.067079 -29.060569 359.278793 0.929892 626 SyXB a. k.a. AX_J1740.2-2903
GRO J1744-28 266.139419 -28.744480 0.042075 0.298489 0.47 11.8 LMXB T "Bursting Pulsar"
GRO J1750-27 267.291434 -26.639700 2.370662 0.518408 4.45 29.82 BeXRB? P aka AX J1749.1-2639
IGR J17544-2619 268.605299 -26.331274 3.235980 -0.335557 4.93 SFXT? C T
SAX J1802.7-2017 270.665728 -20.286816 9.417461 1.044121 139.6 4.57 SG P aka IGR J18027-2016
1RXS J180431.1-273932 271.130284 -27.659214 3.202710 -2.947774 494 SyXB
SAX J1808.4-3658 272.114166 -36.979379 355.384418 -8.148034 0.0025 0.837 LMXB aka V* V4580 Sgr, disk accretor(?)
Swift J1816.7-1613 274.176846 -16.222949 14.587018 0.092428 142.9 151? BeXRB? T ATel 6253 ATel 1457
IGR J18179-1621 274.467048 -16.359400 14.599162 -0.217510 11.82 C? T ATel 3947 ATel 3949
AX J1820.5-1434 275.122921 -14.571809 16.473200 0.070620 152
3A 1822-371 276.445028 -37.105158 356.850238 -11.290768 0.59 0.23 LMXB
Sct X-1 278.857602 -7.614004 24.336027 0.065699 112 111 SyXB
GS 1843+00 281.403474 0.863160 33.036370 1.689359 T
2S 1845-024 282.075590 -2.419729 30.421052 -0.406023 94.8 242.2 BeXRB? T aka GS 1843-02
XTE J1855-026 283.876680 -2.604678 31.076348 -2.092060 361 6.1 SG
XTE J1858+034 284.678379 3.439739 36.822153 -0.048088 221 T
XTE J1859+083 284.778177 8.246352 41.144826 2.058031 9.8 T ATel 7037
4U 1901+03 285.903524 3.190426 37.159966 -1.249760 T
XTE J1906+090 286.197769 9.044912 42.497189 1.174872 89.2 BeXRB?
4U 1907+09 287.408533 9.829777 43.743566 0.475292 441 8.37 SG C P
4U 1909+07 287.700872 7.597657 41.896991 -0.811637 604 4.4 SG P
IGR J19140+0951 288.517606 9.882865 44.296348 -0.468771 13.55 HMXB ?
IGR J19149+1036 288.728311 10.612245 45.038573 -0.313490 22.25 SG C P very close to GRS1915
IGR J19294+1816 292.482927 18.310607 53.540075 0.115022 12.5 116? BeXRB? T
XTE J1946+274 296.413975 27.365400 63.207144 1.395565 15.8 169.2 BeXRB C T
KS 1947+300 297.397839 30.208809 66.098966 2.083585 18.8 40.4 BeXRB C T
3A 1954+319 298.926399 32.096931 68.391941 1.926894 1.91e4 SyXB
EXO 2030+375 308.063627 37.637433 77.151841 -1.241801 41.8 46.03 BeXRB T regular outbursts
GRO J2058+42 314.698059 41.776980 83.569877 -2.655492 T
SAX J2103.5+4545 315.898770 45.751533 87.130252 -0.684802 359 12.7 BeXRB T
IGR J21343+4738 323.584869 47.633380 92.171608 -3.117683 320.35 20.85 BeXRB P? Varying levels of activity
Cep X-4 324.877853 56.986219 99.012209 3.312526 66.32 20.85 BeXRB C T
4U 2206+54 331.984289 54.518433 100.603243 -1.105922 5560 19.25? SG P magnetar?
SAX J2239.3+6116 339.836831 61.274053 107.734431 2.362332 1247 262? BeXRB T
IGR J22534+6243 343.479672 62.726882 109.923864 2.861557 46.7 BeXRB? P?

Location in the Galaxy

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. HEASARC source class identifiers are also given. The spiral arms are from Vallée et al. (2008)[1]. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

Galactic distribution of accreting X-ray pulsars.

# Source Class Dist. [kpc] # Source Class Dist. [kpc]
1 GRO_J1744-28 1490 8.5 33 3A_0656-072 1316 3.9
2 GX_1+4 1410 4.5 34 3A_0726-260 1310 6.1
3 GRO_J1750-27 1316 ? 35 RX_J0812.4-3114 1316 8.8
4 1RXS_J180431.1-273932 1410 ? 36 Ginga_0834-430 1316 4
5 AX_J1820.5-1434 1316 8.2 37 Vela_X-1 1213 1.4
6 XTE_J1855-026 1213 10 38 LMC_X-4 1210 55
7 Sct_X-1 1116 7 39 GRO_J1008-57 1316 5
8 Ginga_1843+009 1316 12.5 40 4U_1036-56 1316 5
9 4U_1901+03 1366 ? 41 Cen_X-3 1263 10
10 4U_1909+07 1210 7 42 1A_1118-615 1366 5
11 XTE_J1906+090 1316 10 43 1E_1145.1-6141 1210 8.5
12 H_1907+097 1216 5 44 H_1145-619 1316 3.1
13 4U_1700+24 1400 0.42 45 GX_301-2 1211 4.1
14 IGR_J19294+1816 1316 ? 46 SMC_X-1 1213 60
15 Her_X-1 1413 6.56 47 3A_1239-599 1110 ?
16 XTE_J1946+274 1316 9.5 48 RX_J0101.8-7223 1310 60
17 KS_1947+300 1316 9.5 49 GX_304-1 1316 2.4
18 3A_1954+319 1416 1.7 50 SAX_J1324.4-6200 1310 10
19 EXO_2030+375 1366 7.1 51 H_1417-624 1316 6
20 GRO_J2058+42 1316 9.0 52 SAX_J1452.8-5949 1010 9
21 SAX_J2103.5+4545 1366 6.8 53 4U_1626-67 1410 9.0
22 Cep_X-4 1316 3.8 54 H_1538-522 1213 6.4
23 3A_2206+543 1260 2.6 55 SWIFT_J1626.6-5156 1366 ?
24 3A_0114+650 1213 4.5 56 AX J1700.1-4157 9999 ?
25 H_0115+634 1386 8 57 OAO_1657-415 1213 7.1
26 IGR_J01583+6713 1316 4 58 IGR_J16358-4726 1110 7
27 RX_J0146.9+6121 1310 2.3 59 IGR_J16393-4643 1210 10.6
28 V_0332+53 1366 7.5 60 IGR_J16194-2810 1400 3.7
29 RX_J0440.9+4431 1310 3.3 61 SAX_J1808.4-3658 1416 3.6
30 X_Per 1310 0.7 62 3A_1822-371 1419 2.5
31 1A_0535+262 1366 2 63 AX_J1740.2-2903 1410 ?
32 SAX_J0635.2+0533 1310 5

The following table describes parallax distances as computed by Bailer-Jones et al. (see this paper and this webpage). Note that these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al. - as an example, the Magellanic cloud sources show up in Gaia DR2 as having distances of ~7 kpc, when they are actually 45 or 60 kpc away.

Source Gaia distance
RX J0101.8-7223 12.3 (+2.0, -1.7)
3A 0114+650 6.6 (+1.6, -1.2)
4U 0115+634 7.2 (+1.5, -1.1)
RX J0146.9+6121 2.50 (+0.22, -0.19)
IGR J01583+6713 7.4 (+1.1, -0.9)
Swift J0243.6+6124 6.9 (+1.6, -1.2)
V 0332+53 5.1 (+1.1, -0.8)
X Per 0.79 +/- 0.04
RX J0440.9+4431 3.2 (+0.7, -0.5)
1A 0535+26 2.13 (+0.26, -0.21)
SAX J0635.2+0533 1.6 (+2.2, -0.8)
MXB 0656-07 5.1 (+1.4, -1.0)
3A 0726-260 9.5 (+3.1, -2.2)
RX J0812.4-3114 6.8 (+1.2, -1.0)
GS 0834-430 5.5 (+2.5, -1.7)
Vela X-1 2.42 (+0.19, -0.17)
4U 1036-56 5.0 (+1.1, -0.8)
1A 1118-616 2.93 (+0.26, -0.22)
Cen X-3 6.4 (+1.4, -1.1)
1E1145.1-6141 9.1 (+2.2, -1.6)
4U 1145-619 2.23 (+0.20, -0.17)
GX 301-2 3.5 (+0.6, -0.5)
3A 1239-599 2.9 (+2.4, -1.3)
GX 304-1 2.01 (+0.15, -0.13)
SAX J1324.4-6200 3.5 (+2.6, -1.7)
2S 1417-624 3.8 (+2.8, -1.8)
SAX J1452.8-5949 3.0 (+2.6, -1.5)
4U 1538-522 6.6 (+2.2, -1.5)
2S 1553-542 3.5 (+2.6, -1.5)
IGR J16194-2810 2.3 (+0.8, -0.5)
Swift J1626.6-5156 9.8 (+3.2, -2.4)
IGR J16318-4848 5.2 (+2.8, -1.9)
IGR J16320-4751 1.3 (+0.6, -0.4)
4U 1626-67 3.5 (+2.3, -1.3)
IGR J16393-4643 4.0 (+2.7, -1.7)
IGR J16465-4507 2.7 (+0.5, -0.4)
Her X-1 5.0 (+0.8, -0.6)
AX J1700.1-4157 3.4 (+2.6, -1.5)
OAO 1657-415 2.2 (+0.7, -0.5)
4U 1700-37 1.75 (+0.24, -0.19)
4U 1700+24 0.536 +/- 0.010
EXO 1722-363 4.0 (+2.3, -1.3)
GX 1+4 7.6 (+4.3, -2.8)
2XMM J174016.0-290337 1.4 (+1.6, -0.5)
GRO J1744-28 1.3 (+1.2, -0.5)
IGR J17544-2619 2.7 (+0.5, -0.4)
SAX J1802.7-2017 1.5 (+2.8, -0.7)
SAX J1808.4-3658 5.1 (+4.3, -2.6)
Swift J1816.7-1613 1.4 (+2.5, -0.7)
3A 1822-371 6.1 (+2.7, -1.6)
GS 1843+00 2.3 (+2.0, -1.0)
XTE J1855-026 8.1 (+2.6, -1.8)
XTE J1858+034 1.55 (+0.28, -0.21)
XTE J1859+083 2.7 (+2.4, -1.5)
4U 1901+03 2.2 (+2.2, -1.3)
XTE J1906+090 2.8 (+2.4, -1.4)
4U 1907+09 4.4 (+2.1, -1.3)
4U 1909+07 2.6 (+2.3, -1.4)
IGR J19140+0951 2.8 (+2.4, -1.4)
IGR J19149+1036 3.0 (+2.5, -1.6)
IGR J19294+1816 2.9 (+2.5, -1.5)
XTE J1946+274 12.6 (+3.9, -2.9)
KS 1947+300 15.2 (+3.7, -2.8)
3A 1954+319 3.3 (+1.0, -0.7)
EXO 2030+375 3.6 (+1.4, -0.9)
GRO J2058+42 8.0 (+1.2, -1.0)
SAX J2103.5+4545 6.4 (+0.9, -0.7)
IGR J21343+4738 7.8 (+1.4, -1.1)
Cep X-4 10.2 (+2.2, -1.6)
4U 2206+54 3.3 +/- 0.4
SAX J2239.3+6116 8.0 (+1.4, -1.1)
IGR J22534+6243 8.1 (+2.3, -1.6)


Correlation between luminosity and CRSF energy

In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page: CRSF energy as function of luminosity

Assignments

Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. The list can only be accessed if logged in.

  1. ↑ Vallée, Jacques P., 2008, ApJ 681, 303 (NASA ADS)
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