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

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(Added a first draft of a table of Gaia distances to a selection of sources.)
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== ''Gaia'' distances for selected sources ==
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These distances are based on ''Gaia'' DR2 and are from [http://www.mpia.de/homes/calj/gdr2_distances/main.html].
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{| class="wikitable"
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! Name
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! Gaia ID
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! Distance (kpc)
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|-
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| 2S 0114+650 || 524924310153249920 || 6.562587 (+1.116711, -1.566287)
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|-
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| 4U 0115+634 || 524677469790488960 || 7.199713 (+1.095894, -1.475555)
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|-
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| SWIFT J0243.6+6124 || 465628193526364416 || 6.855165 (+1.113569, -1.528309)
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|-
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| V 0332+53 || 444752973131169664 || 5.133034 (+0.758969, -1.017930)
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|-
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| X Per || 168450545792009600 || 0.792549 (+0.034039, -0.037171)
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|-
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| RX J0440.9+4431 || 252878401557369088 || 3.249340 (+0.454437, -0.615667)
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|-
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| 1A 0535+262 || 3441207615229815040 || 2.126258 (+0.208209, -0.257085)
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|-
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| XTE J0658-073 || 3052677318793446016 || 5.114345 (+0.929704, -1.352583)
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|-
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| Vela X-1 || 5620657678322625920 || 2.415107 (+0.164245, -0.189298)
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|-
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| 1A 1118-615 || 5336957010898124160 || 2.925149 (+0.218751, -0.256124)
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| Cen X-3 || 5337498593446516480 || 6.368538 (+1.005686, -1.390803)
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| GX 301-2 || 6054569565614460800 || 3.532362 (+0.403017, -0.515782)
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| GX 304-1 || 5863533199843070208 || 2.010822 (+0.127915, -0.146118)
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|-
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| 4U 1538-522 || 5886085557746480000 || 6.647552 (+1.439119, -2.109515)
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| Her X-1 || 1338822021487330304 || 5.038977 (+0.566184, -0.706038)
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|-
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| 4U 1700-37 || 5976382915813535232 || 1.749404 (+0.185869, -0.234553)
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|-
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| IGR J17544-2619 || 4063908810076415872 || 2.660014 (+0.333967, -0.441861)
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|-
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| 2A 1822-371 || 6728016172687965568 || 6.052942 (+1.570159, -2.680451)
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|-
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| 4U 1907+09 || 4309225217336729088 || 4.389187 (+1.223733, -2.009640)
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|-
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| EXO 2030+375 || 2063791369815322752 || 3.636518 (+0.882025, -1.342077)
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|-
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| Cep X-4 || 2178178409188167296 || 10.167831 (+1.593317, -2.140719)
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|-
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| 4U 2206+54 || 2005653524280214400 || 3.344543 (+0.315553, -0.385478)
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|-
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|}
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= Correlation between luminosity and CRSF energy =
 
= Correlation between luminosity and CRSF energy =

Revision as of 15:40, 8 July 2018


Source l b Pspin [s] Porbital [d] System CRSF? Notes
GRO J1744-28 0.05 +0.30 0.47 11.8 LMXB T "Bursting Pulsar"
GX 1+4 1.94 +4.79 170 1161 SyXB P Pspin evolving rapidly
GRO J1750-27 2.37 +0.51 4.45 29.82 BeXRB? P a.k.a. AX J1749.1-2639
1RXS J180431.1-273932 3.20 -2.95 494 SyXB
SAX J1802.7-2017 9.42 +1.04 139.6 4.57 SG P a.k.a. IGR J18027-2016
Swift J1816.7-1613 14.59 +0.09 142.9 151? BeXRB? T ATel 6253 ATel 1457
IGR J18179-1621 14.60 -0.22 11.82 C? T ATel 3947 ATel 3949
AX J1820.5-1434 16.47 +0.07 152 ? ?
Sct X-1 24.34 +0.07 112 111 SyXB
2S 1845-024 30.42 -0.4 94.8 242.2 BeXRB? T a.k.a. GS 1843-02
XTE J1855-026 31.07 -2.09 361 6.1 SG
GS 1843+00 33.04 +1.69 T
XTE J1858+034 36.82 -0.06 221 T
4U 1901+03 37.16 -1.25 T
XTE J1859+083 41.15 +2.06 9.8 T ATel 7037
4U 1909+07 41.90 -0.81 604 4.4 SG P
XTE J1906+090 42.59 +0.89 89.2 BeXRB?
4U 1907+09 43.74 +0.48 441 8.37 SG C P
IGR J19140+0951 44.30 -0.47 13.55 HMXB ?
4U 1700+24 45.15 +32.99 404 SyXB
IGR J19294+1816 53.44 +0.20 12.5 116? BeXRB? T
Her X-1 58.15 +37.5 1.24 1.7 IM C P
XTE J1946+274 63.21 +1.40 15.8 169.2 BeXRB C T
KS 1947+300 66.10 +2.08 18.8 40.4 BeXRB C T
3A 1954+319 68.39 +1.93 1.91e4 SyXB
EXO 2030+375 77.15 -1.24 41.8 46.03 BeXRB T regular outbursts
GRO J2058+42 83.55 -2.72 T
SAX J2103.5+4545 87.12 +0.68 359 12.7 BeXRB T
IGR J21343+4738 92.17 -3.12 320.35 20.85 BeXRB P? Varying levels of activity
Cep X-4 99.01 +3.31 66.32 20.85 BeXRB C T
4U 2206+54 100.6 -1.11 5560 19.25? SG P magnetar?
SAX J2239.3+6116 107.7 +2.36 1247 262? BeXRB T
IGR J22534+6243 109.92 +2.86 46.7 Be? P?
3A 0114+650 125.71 +2.56 9828 11.6 SG P 30.7 d superorbital modulation
4U 0115+634 125.92 +1.03 3.6 24.3 BeXRB C T 5 or more lines
IGR J01583+6713 129.4 +5.19 469? BeXRB C? T controversial claim of CRSF features
RX J0146.9+6121 129.54 -0.80 1412 330? BeXRB T a.k.a. V* V831 Cas
V 0332+53 146.05 -2.19 4.37 34.25 BeXRB C T multiple lines
RX J0440.9+4431 159.9 -1.27 203 155 BeXRB P a.k.a. LS V+44 17, persistent, but with outbursts
X Per 163.1 -17.1 830 250.3 BeXRB C? P magnetar?
A0535+26 181.5 -2.64 103 111.1 BeXRB C T
SAX J0635.2+0533 206.15 -1.04 0.0338 BeXRB T low luminosity
MXB 0656-07 220.13 -1.77 160.4 101.2 BeXRB C a.k.a XTE J0658-073
3A 0726-260 240.3 -4.05 103.2 34.5 BeXRB T
RX J0812.4-3114 249.6 +1.54 31.9 80 BeXRB T
GS 0834-430 262.02 -1.51 12.3 105.8 BeXRB T
Vela X-1 263.06 +3.9 283 8.96 SG C P eclipsing
LMC X-4 276.3 -32.5 13.5 1.4 SG P superorbital variation ~30 d
Swift  J053041.9-665426 277.0 -32.7 28.78 BeXRB T?
LXP 169 279.2 -34.5 168.8 24.3 BeXRB T? NS eclipsing companion
GRO J1008-57 283.0 -1.83 93.7 249.48 BeXRB C? T outbursts predicted precisely
4U 1036-56 285.36 +1.43 862 BeXRB P? a.k.a. RX J1037.5-564/LS 1698
IGR J19149+1036 288.736 +10.611 22.25 SG C P very close to GRS1915
Cen X-3 292.09 +0.34 4.8 2.09 SG C P disk-fed HMXB
1A 1118-616 292.5 -0.89 407 24? BeXRB C T
1E1145.1-6141 295.5 -0.01 297 14.4 SG (V* V830 Cen) varying luminosity states
4U 1145-619 295.6 -0.24 292 187.5 BeXRB PT
SXP 265 299.2 -42.4 264.52 ~146 BeXRB PT SMC region, persistent low luminosity, one type I outburst
GX 301-2 300.1 -0.04 686 41.5 SG C P very massive companion, strong orbital variability
SMC X-1 300.4 -43.6 0.71 3.892 SG P eclipsing
3A 1239-599 301.8 +2.6 191
RX J0101.8-7223 301.8 -44.7 175 BeXRB T
RX J0059.2-7138 302.1 -45.5 2.76 82d? BeXRB? C? T a.k.a SXP 2.76
CXOU J005047.9-731817 303.0 -43.8 292 BeXRB? T
GX 304-1 304.1 +1.25 272 132.2 BeXRB C T Strong spectral parameter variations
SAX J1324.4-6200 306.8 +0.61 171 22 BeXRB?
2S 1417-624 313.0 -1.60 17.6 42.12 BeXRB T
SAX J1452.8-5949 317.6 -0.46 437 BeXRB?
4U 1626-67 321.8 -13.1 7.7 0.029 WD? C Torque reversals
4U 1538-52 327.4 +2.16 530 3.7 SG C P
2S 1553-542 327.9 -0.86 9.3 29.56 BeXRB? P Occasional outbursts
Swift J1626.6-5156 332.8 -2.00 15.4 132.9 BeXRB C T strong flares
IGR J16318-4848 335.616 -0.4477 SG P super absorbed source
IGR J16320-4751 336.3297 +0.1688 1309 8.986 SG P aka 2FGL J1632.4-4753c
IGR J16358-4726 337.1 -0.01 5880 SyXB
IGR J16393-4643 338.0 +0.07 912 3.7 SyXB a.k.a. AX J1639.0-4642
IGR J16465-4507 340.0535 +0.135 228 30.243 P aka 2MASS J16463526-4507045
AX J1700.1-4157 344.0 +0.24 715 BeXRB?
OAO 1657-415 344.4 +0.31 37.7 10.4 SG C? P eclipsing
IGR J16194-2810 349.1 +15.5 SyXB
EXO 1722-363 351.5 -0.35 ~414 9.74 HMXB a.k.a. IGR J17252–3616, heavily absorbed, eclipsing
SAX J1808.4-3658 355.4 -8.15 0.0025 0.837 LMXB a.k.a. V* V4580 Sgr, disk accretor(?)
3A 1822-371 356.85 -11.29 0.59 0.23 LMXB
2XMM J174016.0−290337 359.3 +0.93 626 ? SyXB a. k.a. AX_J1740.2-2903


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

Gaia distances for selected sources

These distances are based on Gaia DR2 and are from [1].

Name Gaia ID Distance (kpc)
2S 0114+650 524924310153249920 6.562587 (+1.116711, -1.566287)
4U 0115+634 524677469790488960 7.199713 (+1.095894, -1.475555)
SWIFT J0243.6+6124 465628193526364416 6.855165 (+1.113569, -1.528309)
V 0332+53 444752973131169664 5.133034 (+0.758969, -1.017930)
X Per 168450545792009600 0.792549 (+0.034039, -0.037171)
RX J0440.9+4431 252878401557369088 3.249340 (+0.454437, -0.615667)
1A 0535+262 3441207615229815040 2.126258 (+0.208209, -0.257085)
XTE J0658-073 3052677318793446016 5.114345 (+0.929704, -1.352583)
Vela X-1 5620657678322625920 2.415107 (+0.164245, -0.189298)
1A 1118-615 5336957010898124160 2.925149 (+0.218751, -0.256124)
Cen X-3 5337498593446516480 6.368538 (+1.005686, -1.390803)
GX 301-2 6054569565614460800 3.532362 (+0.403017, -0.515782)
GX 304-1 5863533199843070208 2.010822 (+0.127915, -0.146118)
4U 1538-522 5886085557746480000 6.647552 (+1.439119, -2.109515)
Her X-1 1338822021487330304 5.038977 (+0.566184, -0.706038)
4U 1700-37 5976382915813535232 1.749404 (+0.185869, -0.234553)
IGR J17544-2619 4063908810076415872 2.660014 (+0.333967, -0.441861)
2A 1822-371 6728016172687965568 6.052942 (+1.570159, -2.680451)
4U 1907+09 4309225217336729088 4.389187 (+1.223733, -2.009640)
EXO 2030+375 2063791369815322752 3.636518 (+0.882025, -1.342077)
Cep X-4 2178178409188167296 10.167831 (+1.593317, -2.140719)
4U 2206+54 2005653524280214400 3.344543 (+0.315553, -0.385478)


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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