Difference between revisions of "List of accreting X-ray pulsars"
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= List of accreting X-ray pulsars = | = List of accreting X-ray pulsars = | ||
{| class="wikitable" | {| class="wikitable" | ||
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! Source | ! Source | ||
− | ! | + | ! RA |
− | ! | + | ! Dec |
− | ! | + | ! Distance (kpc) |
− | ! | + | ! Pspin (s) |
− | ! | + | ! Porbit (d) |
+ | ! Type | ||
! CRSF? | ! CRSF? | ||
− | ! | + | ! Persistent? |
! Notes | ! Notes | ||
+ | |- | ||
+ | | [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 60 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292 | ||
+ | |- | ||
+ | |||
+ | | [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 60 || 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) || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T || |
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− | | [[ | + | | [[SMC X-1]] || 19.271456 || -73.443343 || 60 || 0.71 || 3.892 || SG || || P || eclipsing |
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− | | P | ||
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− | | [[ | + | | [[3A 0114+650]] || 19.511228 || 65.291623 || 4.5 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation |
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− | | P | ||
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− | | [[ | + | | [[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 |
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− | | | + | | [[SXP 265]] || 23.214439 || -74.429258 || 60 || 264.52 || || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst |
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− | | [[List of | ||
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[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? |
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[X Per]] || 58.846151 || 31.045836 || 0.79 +/- 0.04 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || || P || magnetar? |
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− | | [[List of | ||
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− | | [[ | + | | [[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 |
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− | | BeXRB | ||
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− | | [[ | + | | [[LXP 169]] || 76.981153 || -68.418135 || 45 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion, LMC source |
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− | | [[ | + | | [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 45 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? || LMC source |
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− | | [[ | + | | [[LMC X-4]] || 83.206501 || -66.370332 || 45 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d |
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− | | [[ | + | | [[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 || |
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[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 || |
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− | | BeXRB | ||
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− | | [[ | + | | [[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 || |
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− | | [[List of | ||
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− | | [[ | + | | [[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 || |
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[GRO J1008-57]] || 152.439620 || -58.292035 || 5 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely |
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− | | BeXRB? | ||
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[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 || |
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− | | [[List of Be X-ray Binaries|BeXRB]] | ||
− | | [[List of cyclotron line sources|C]] | ||
− | | T | ||
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− | | [[ | + | | [[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 |
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− | | [[List of cyclotron line sources|C]] | ||
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− | | [[ | + | | [[1E1145.1-6141]] || 176.868942 || -61.953720 || 9.1 (+2.2, -1.6) || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states |
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− | | [[ | + | | [[4U 1145-619]] || 177.000032 || -62.206910 || 2.23 (+0.20, -0.17) || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT || |
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[3A 1239-599]] || 190.508997 || -60.200951 || 2.9 (+2.4, -1.3) || 191 || || || || || |
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 3.5 (+2.6, -1.7) || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || || |
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− | | [[ | + | | [[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 || |
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− | | [[SAX | + | | [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 3.0 (+2.6, -1.5) || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || || |
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− | | [[ | + | | [[4U 1538-522]] || 235.597300 || -52.386011 || 6.6 (+2.2, -1.5) || 526 || 3.72 || SG || [[List of cyclotron line sources|C]] || P || |
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− | | [[ | + | | [[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 |
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− | | +2.56 | ||
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− | | [[ | + | | [[IGR J16194-2810]] || 244.888926 || -28.127773 || 2.3 (+0.8, -0.5) || || || [[List of symbiotic X-ray binaries|SyXB]] || || || |
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[IGR J16318-4848]] || 247.951259 || -48.816876 || 5.2 (+2.8, -1.9) || || || SG || || P || super absorbed source |
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− | | [[ | + | | [[IGR J16320-4751]] || 248.009669 || -47.874785 || 1.3 (+0.6, -0.4) || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c |
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− | | [[ | + | | [[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. |
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− | | [[ | + | | [[IGR J16358-4726]] || 249.124997 || -47.623903 || 7 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || || |
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[IGR J16465-4507]] || 251.646902 || -45.117960 || 2.7 (+0.5, -0.4) || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045 |
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− | | [[ | + | | [[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 || |
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− | | [[List of cyclotron line sources|C]] | ||
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− | | [[ | + | | [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 3.4 (+2.6, -1.5) || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || || |
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[4U 1700-37]] || 255.986566 || -37.844121 || 1.75 (+0.24, -0.19) || || 3.4 || SG || || P || No pulsations, eclipsing source |
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− | | [[ | + | | [[4U 1700+24]] || 256.643762 || 23.971820 || 0.536 +/- 0.010 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || || |
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[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 |
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− | | [[ | + | | [[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 |
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− | | [[GRO | + | | [[GRO J1744-28]] || 266.139419 || -28.744480 || 1.3 (+1.2, -0.5) || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar" |
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− | | [[ | + | | [[GRO J1750-27]] || 267.291434 || -26.639700 || || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || a.k.a. AX J1749.1-2639 |
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− | | [[List of Be X-ray Binaries|BeXRB]] | ||
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− | | [[IGR | + | | [[IGR J17544-2619]] || 268.605299 || -26.331274 || 2.7 (+0.5, -0.4) || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T || |
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− | | [[ | + | | [[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 |
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|- | |- | ||
− | | [[ | + | | [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || || |
− | | | ||
− | | - | ||
− | | | ||
− | | | ||
− | | [[List of | ||
− | | | ||
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− | | | ||
|- | |- | ||
− | | [[ | + | | [[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(?) |
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
|- | |- | ||
− | | [[ | + | | [[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] |
− | | | ||
− | | -0. | ||
− | | | ||
− | | | ||
− | | [[List of Be X-ray Binaries|BeXRB]] | ||
− | | | ||
− | | | ||
− | | | ||
|- | |- | ||
− | | [[ | + | | [[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] |
− | | | ||
− | | - | ||
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− | | | ||
|- | |- | ||
− | | [[ | + | | [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 8.2 || 152 || || ? || || ? || |
− | | | ||
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− | | | ||
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|- | |- | ||
− | | [[ | + | | [[3A 1822-371]] || 276.445028 || -37.105158 || 6.1 (+2.7, -1.6) || 0.59 || 0.23 || LMXB || || || |
− | | | ||
− | | - | ||
− | | | ||
− | | | ||
− | | | ||
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|- | |- | ||
− | | [[ | + | | [[Sct X-1]] || 278.857602 || -7.614004 || 7.5 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || || |
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
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|- | |- | ||
− | | [[ | + | | [[GS 1843+00]] || 281.403474 || 0.863160 || 2.3 (+2.0, -1.0) || || || || || T || |
− | | | ||
− | | - | ||
− | | | ||
− | | | ||
− | | | ||
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|- | |- | ||
− | | [[ | + | | [[2S 1845-024]] || 282.075590 || -2.419729 || || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || a.k.a. GS 1843-02 |
− | | | ||
− | | - | ||
− | | | ||
− | | | ||
− | | BeXRB? | ||
− | | | ||
− | | T | ||
− | | a.k.a | ||
|- | |- | ||
− | | [[ | + | | [[XTE J1855-026]] || 283.876680 || -2.604678 || 8.1 (+2.6, -1.8) || 361 || 6.1 || SG || || || |
− | | | ||
− | | - | ||
− | | | ||
− | | | ||
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|- | |- | ||
− | | [[ | + | | [[XTE J1858+034]] || 284.678379 || 3.439739 || 1.55 (+0.28, -0.21) || || 221 || || || T || |
− | | | ||
− | |||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | 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] |
− | | | ||
− | | + | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
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|- | |- | ||
− | | [[ | + | | [[4U 1901+03]] || 285.903524 || 3.190426 || 2.2 (+2.2, -1.3) || || || || || T || |
− | | | ||
− | | -1. | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | T | ||
− | | | ||
|- | |- | ||
− | | [[ | + | | [[XTE J1906+090]] || 286.197769 || 9.044912 || 2.8 (+2.4, -1.4) || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || || |
− | | | ||
− | | - | ||
− | | | ||
− | | | ||
− | | BeXRB? | ||
− | | | ||
− | | | ||
− | | | ||
|- | |- | ||
− | | [[4U | + | | [[4U 1907+09]] || 287.408533 || 9.829777 || 4.4 (+2.1, -1.3) || 442 || 8.37 || SG || [[List of cyclotron line sources|C]] || P || |
− | | | ||
− | | - | ||
− | | | ||
− | | | ||
− | | | ||
− | | [[List of cyclotron line sources|C]] | ||
− | | | ||
− | | | ||
|- | |- | ||
− | | [[4U | + | | [[4U 1909+07]] || 287.700872 || 7.597657 || 2.6 (+2.3, -1.4) || 604 || 4.4 || SG || || P || |
− | | | ||
− | | +2. | ||
− | | | ||
− | | | ||
− | | SG | ||
− | | | ||
− | | P | ||
− | | | ||
|- | |- | ||
− | | [[ | + | | [[IGR J19140+0951]] || 288.517606 || 9.882865 || 2.8 (+2.4, -1.4) || || 13.55 || HMXB || || ? || |
− | | | ||
− | | - | ||
− | | | ||
− | | | ||
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|- | |- | ||
− | | [[ | + | | [[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 |
− | | | ||
− | | - | ||
− | | | ||
− | | | ||
− | | | ||
− | | [[List of cyclotron line sources|C]] | ||
− | | | ||
− | | | ||
|- | |- | ||
− | | [[IGR | + | | [[IGR J19294+1816]] || 292.482927 || 18.310607 || 2.9 (+2.5, -1.5) || 12.5 || 116 || [[List of Be X-ray Binaries|BeXRB]]? || || T || |
− | | | ||
− | | - | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
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|- | |- | ||
− | | [[ | + | | [[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 || |
− | | | ||
− | | + | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
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− | | | ||
|- | |- | ||
− | | [[ | + | | [[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 || |
− | | | ||
− | | - | ||
− | | | ||
− | | | ||
− | | [[List of | ||
− | | | ||
− | | | ||
− | | | ||
|- | |- | ||
− | | [[ | + | | [[3A 1954+319]] || 298.926399 || 32.096931 || 3.3 (+1.0, -0.7) || 19100 || || [[List of symbiotic X-ray binaries|SyXB]] || || || |
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | [[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 |
− | | | ||
− | | +0. | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
− | | | ||
|- | |- | ||
− | | [[ | + | | [[GRO J2058+42]] || 314.698059 || 41.776980 || 8.0 (+1.2, -1.0) || || || || || T || |
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− | |||
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|- | |- | ||
− | | [[ | + | | [[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 || |
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− | |||
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|- | |- | ||
− | | [[IGR | + | | [[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 |
− | | | ||
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− | | | ||
− | | | ||
− | | [[List of | ||
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|- | |- | ||
− | | [[ | + | | [[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 || |
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− | | - | ||
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|- | |- | ||
− | | [[ | + | | [[4U 2206+54]] || 331.984289 || 54.518433 || 3.3 +/- 0.4 || 5560 || 19.25 || SG || || P || magnetar? |
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|- | |- | ||
− | | [[ | + | | [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 8.0 (+1.4, -1.1) || 1247 || 262 || [[List of Be X-ray Binaries|BeXRB]] || || T || |
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|- | |- | ||
− | | [[ | + | | [[IGR J22534+6243]] || 343.479672 || 62.726882 || 8.1 (+2.3, -1.6) || 46.7 || || Be? || || P? || |
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|} | |} | ||
+ | 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. | ||
Line 1,279: | Line 617: | ||
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= Correlation between luminosity and CRSF energy = | = Correlation between luminosity and CRSF energy = |
Revision as of 23:01, 10 July 2018
List of accreting X-ray pulsars
Source | RA | Dec | Distance (kpc) | Pspin (s) | Porbit (d) | Type | CRSF? | Persistent? | Notes |
---|---|---|---|---|---|---|---|---|---|
CXOU J005047.9-731817 | 12.699963 | -73.305018 | 60 | 292 | BeXRB? | T | aka SXP 292 | ||
RX J0059.2-7138 | 14.803112 | -71.645828 | 60 | 2.76 | 82 | BeXRB? | C? | T | aka SXP 2.76 |
RX J0101.8-7223 | 15.467910 | -72.392796 | 12.3 (+2.0, -1.7) | 175 | BeXRB | T | |||
SMC X-1 | 19.271456 | -73.443343 | 60 | 0.71 | 3.892 | SG | P | eclipsing | |
3A 0114+650 | 19.511228 | 65.291623 | 4.5 | 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 | BeXRB | C | T | 5 or more lines |
SXP 265 | 23.214439 | -74.429258 | 60 | 264.52 | 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 | BeXRB | T | a.k.a. V* V831 Cas | |
IGR J01583+6713 | 29.577033 | 67.223185 | 7.4 (+1.1, -0.9) | 469 | BeXRB | 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 | BeXRB | T | Galactic ULX? | |
V 0332+53 | 53.749630 | 53.173140 | 5.1 (+1.1, -0.8) | 4.37 | 34.25 | BeXRB | C | T | multiple lines |
X Per | 58.846151 | 31.045836 | 0.79 +/- 0.04 | 830 | 250.3 | BeXRB | P | magnetar? | |
RX J0440.9+4431 | 70.247207 | 44.530344 | 3.2 (+0.7, -0.5) | 203 | 155 | BeXRB | P | a.k.a. LS V+44 17, persistent, but with outbursts | |
LXP 169 | 76.981153 | -68.418135 | 45 | 168.8 | 24.3 | BeXRB | T? | NS eclipsing companion, LMC source | |
Swift J053041.9-665426 | 82.675788 | -66.907566 | 45 | 28.78 | BeXRB | T? | LMC source | ||
LMC X-4 | 83.206501 | -66.370332 | 45 | 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 | BeXRB | C | T | |
SAX J0635.2+0533 | 98.822528 | 5.553870 | 1.6 (+2.2, -0.8) | 0.0338 | BeXRB | T | low luminosity | ||
MXB 0656-07 | 104.572030 | -7.209774 | 5.1 (+1.4, -1.0) | 160.4 | 101.2 | BeXRB | C | a.k.a XTE J0658-073 | |
3A 0726-260 | 112.223241 | -26.108019 | 9.5 (+3.1, -2.2) | 103.2 | 34.5 | BeXRB | T | ||
RX J0812.4-3114 | 123.118149 | -31.247807 | 6.8 (+1.2, -1.0) | 31.9 | 80 | BeXRB | T | ||
GS 0834-430 | 128.981072 | -43.185598 | 5.5 (+2.5, -1.7) | 12.3 | 105.8 | BeXRB | T | ||
Vela X-1 | 135.528560 | -40.554654 | 2.42 (+0.19, -0.17) | 283 | 8.96 | SG | C | P | eclipsing |
GRO J1008-57 | 152.439620 | -58.292035 | 5 | 93.7 | 249.48 | BeXRB | C? | T | outbursts predicted precisely |
4U 1036-56 | 159.397094 | -56.798840 | 5.0 (+1.1, -0.8) | 862 | BeXRB | P? | a.k.a. RX J1037.5-564/LS 1698 | ||
1A 1118-616 | 170.238174 | -61.916707 | 2.93 (+0.26, -0.22) | 407 | 24 | BeXRB | C | T | |
Cen X-3 | 170.312856 | -60.623776 | 6.4 (+1.4, -1.1) | 4.8 | 2.09 | SG | 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 | ||
4U 1145-619 | 177.000032 | -62.206910 | 2.23 (+0.20, -0.17) | 292 | 187.5 | BeXRB | PT | ||
GX 301-2 | 186.656453 | -62.770359 | 3.5 (+0.6, -0.5) | 686 | 41.5 | SG | C | P | very massive companion, strong orbital variability |
3A 1239-599 | 190.508997 | -60.200951 | 2.9 (+2.4, -1.3) | 191 | |||||
GX 304-1 | 195.321198 | -61.601845 | 2.01 (+0.15, -0.13) | 272 | 132.2 | BeXRB | C | T | Strong spectral parameter variations |
SAX J1324.4-6200 | 201.108853 | -62.016515 | 3.5 (+2.6, -1.7) | 171 | 22 | BeXRB? | |||
2S 1417-624 | 215.303896 | -62.698168 | 3.8 (+2.8, -1.8) | 17.6 | 42.12 | BeXRB | T | ||
SAX J1452.8-5949 | 223.207002 | -59.820983 | 3.0 (+2.6, -1.5) | 437 | BeXRB? | ||||
4U 1538-522 | 235.597300 | -52.386011 | 6.6 (+2.2, -1.5) | 526 | 3.72 | SG | C | P | |
2S 1553-542 | 239.452345 | -54.416113 | 3.5 (+2.6, -1.5) | 9.3 | 29.56 | BeXRB? | P | Occasional outbursts | |
IGR J16194-2810 | 244.888926 | -28.127773 | 2.3 (+0.8, -0.5) | SyXB | |||||
Swift J1626.6-5156 | 246.652146 | -51.941848 | 9.8 (+3.2, -2.4) | 15.4 | 132.9 | BeXRB | C | T | strong flares |
IGR J16318-4848 | 247.951259 | -48.816876 | 5.2 (+2.8, -1.9) | 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 | |
4U 1626-67 | 248.069509 | -67.461207 | 3.5 (+2.3, -1.3) | 7.7 | 0.029 | WD? | C | Torque reversals. Only UCXB with a CRSF. | |
IGR J16358-4726 | 249.124997 | -47.623903 | 7 | 5880 | SyXB | ||||
IGR J16393-4643 | 249.772382 | -46.704006 | 4.0 (+2.7, -1.7) | 912 | 3.7 | SyXB | a.k.a. 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 | ||
Her X-1 | 254.457539 | 35.342324 | 5.0 (+0.8, -0.6) | 1.24 | 1.7 | IMXB | C | P | |
AX J1700.1-4157 | 255.018132 | -41.968217 | 3.4 (+2.6, -1.5) | 715 | BeXRB? | ||||
OAO 1657-415 | 255.202665 | -41.654882 | 2.2 (+0.7, -0.5) | 37.7 | 10.4 | SG | 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+24 | 256.643762 | 23.971820 | 0.536 +/- 0.010 | 404 | 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 | |||
GX 1+4 | 263.008955 | -24.745600 | 7.6 (+4.3, -2.8) | 170 | 1161 | SyXB | P | Pulse period evolving rapidly | |
2XMM J174016.0-290337 | 265.067079 | -29.060569 | 1.4 (+1.6, -0.5) | 626 | 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 J1750-27 | 267.291434 | -26.639700 | 4.45 | 29.82 | BeXRB? | P | a.k.a. AX J1749.1-2639 | ||
IGR J17544-2619 | 268.605299 | -26.331274 | 2.7 (+0.5, -0.4) | 4.93 | SFXT? | 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 | |
1RXS J180431.1-273932 | 271.130284 | -27.659214 | 494 | 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(?) | ||
Swift J1816.7-1613 | 274.176846 | -16.222949 | 1.4 (+2.5, -0.7) | 142.9 | 151 | BeXRB? | T | ATel 6253 ATel 1457 | |
IGR J18179-1621 | 274.467048 | -16.359400 | 11.82 | C? | T | ATel 3947 ATel 3949 | |||
AX J1820.5-1434 | 275.122921 | -14.571809 | 8.2 | 152 | ? | ? | |||
3A 1822-371 | 276.445028 | -37.105158 | 6.1 (+2.7, -1.6) | 0.59 | 0.23 | LMXB | |||
Sct X-1 | 278.857602 | -7.614004 | 7.5 | 112 | 111 | SyXB | |||
GS 1843+00 | 281.403474 | 0.863160 | 2.3 (+2.0, -1.0) | T | |||||
2S 1845-024 | 282.075590 | -2.419729 | 94.8 | 242.2 | BeXRB? | T | a.k.a. GS 1843-02 | ||
XTE J1855-026 | 283.876680 | -2.604678 | 8.1 (+2.6, -1.8) | 361 | 6.1 | SG | |||
XTE J1858+034 | 284.678379 | 3.439739 | 1.55 (+0.28, -0.21) | 221 | T | ||||
XTE J1859+083 | 284.778177 | 8.246352 | 2.7 (+2.4, -1.5) | 9.8 | T | ATel 7037 | |||
4U 1901+03 | 285.903524 | 3.190426 | 2.2 (+2.2, -1.3) | T | |||||
XTE J1906+090 | 286.197769 | 9.044912 | 2.8 (+2.4, -1.4) | 89.2 | BeXRB? | ||||
4U 1907+09 | 287.408533 | 9.829777 | 4.4 (+2.1, -1.3) | 442 | 8.37 | SG | C | P | |
4U 1909+07 | 287.700872 | 7.597657 | 2.6 (+2.3, -1.4) | 604 | 4.4 | SG | P | ||
IGR J19140+0951 | 288.517606 | 9.882865 | 2.8 (+2.4, -1.4) | 13.55 | HMXB | ? | |||
IGR J19149+1036 | 288.728311 | 10.612245 | 3.0 (+2.5, -1.6) | 22.25 | SG | C | P | very close to GRS1915 | |
IGR J19294+1816 | 292.482927 | 18.310607 | 2.9 (+2.5, -1.5) | 12.5 | 116 | BeXRB? | T | ||
XTE J1946+274 | 296.413975 | 27.365400 | 12.6 (+3.9, -2.9) | 15.8 | 169.2 | BeXRB | C | T | |
KS 1947+300 | 297.397839 | 30.208809 | 15.2 (+3.7, -2.8) | 18.8 | 40.4 | BeXRB | C | T | |
3A 1954+319 | 298.926399 | 32.096931 | 3.3 (+1.0, -0.7) | 19100 | SyXB | ||||
EXO 2030+375 | 308.063627 | 37.637433 | 3.6 (+1.4, -0.9) | 41.8 | 46.03 | BeXRB | T | regular outbursts | |
GRO J2058+42 | 314.698059 | 41.776980 | 8.0 (+1.2, -1.0) | T | |||||
SAX J2103.5+4545 | 315.898770 | 45.751533 | 6.4 (+0.9, -0.7) | 359 | 12.7 | BeXRB | T | ||
IGR J21343+4738 | 323.584869 | 47.633380 | 7.8 (+1.4, -1.1) | 320.35 | 20.85 | BeXRB | P? | Varying levels of activity | |
Cep X-4 | 324.877853 | 56.986219 | 10.2 (+2.2, -1.6) | 66.32 | 20.85 | BeXRB | C | T | |
4U 2206+54 | 331.984289 | 54.518433 | 3.3 +/- 0.4 | 5560 | 19.25 | SG | P | magnetar? | |
SAX J2239.3+6116 | 339.836831 | 61.274053 | 8.0 (+1.4, -1.1) | 1247 | 262 | BeXRB | T | ||
IGR J22534+6243 | 343.479672 | 62.726882 | 8.1 (+2.3, -1.6) | 46.7 | Be? | P? |
Distances with uncertainties are from Gaia data release 2, as described by Bailer-Jones et al. (see this paper and 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
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.
# | 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 |
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.