Difference between revisions of "List of accreting X-ray pulsars"
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| 8.37 | | 8.37 | ||
| SG | | SG | ||
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| P | | P | ||
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| 404 | | 404 | ||
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| 1.7 | | 1.7 | ||
| IM | | IM | ||
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| P | | P | ||
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| 15.8 | | 15.8 | ||
| 169.2 | | 169.2 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| T | | T | ||
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| 18.8 | | 18.8 | ||
| 40.4 | | 40.4 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| T | | T | ||
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Line 283: | Line 283: | ||
| 1.91e4 | | 1.91e4 | ||
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Line 294: | Line 294: | ||
| 41.8 | | 41.8 | ||
| 46.03 | | 46.03 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
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| T | | T | ||
Line 316: | Line 316: | ||
| 359 | | 359 | ||
| 12.7 | | 12.7 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
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| T | | T | ||
Line 327: | Line 327: | ||
| 320.35 | | 320.35 | ||
| 20.85 | | 20.85 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
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| P? | | P? | ||
Line 338: | Line 338: | ||
| 66.32 | | 66.32 | ||
| 20.85 | | 20.85 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| T | | T | ||
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Line 393: | Line 393: | ||
| 3.6 | | 3.6 | ||
| 24.3 | | 24.3 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| T | | T | ||
| 5 or more lines | | 5 or more lines | ||
Line 404: | Line 404: | ||
| 469? | | 469? | ||
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− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
| C? | | C? | ||
| T | | T | ||
Line 415: | Line 415: | ||
| 1412 | | 1412 | ||
| 330? | | 330? | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
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| T | | T | ||
Line 426: | Line 426: | ||
| 4.37 | | 4.37 | ||
| 34.25 | | 34.25 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| T | | T | ||
| multiple lines | | multiple lines | ||
Line 437: | Line 437: | ||
| 203 | | 203 | ||
| 155 | | 155 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
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| P | | P | ||
Line 448: | Line 448: | ||
| 830 | | 830 | ||
| 250.3 | | 250.3 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
− | | [[ | + | | [[List of cyclotron line sources|C]]? |
| P | | P | ||
| magnetar? | | magnetar? | ||
Line 459: | Line 459: | ||
| 103 | | 103 | ||
| 111.1 | | 111.1 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| T | | T | ||
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Line 470: | Line 470: | ||
| 0.0338 | | 0.0338 | ||
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− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
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| T | | T | ||
Line 481: | Line 481: | ||
| 160.4 | | 160.4 | ||
| 101.2 | | 101.2 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| | | | ||
| a.k.a XTE J0658-073 | | a.k.a XTE J0658-073 | ||
Line 492: | Line 492: | ||
| 103.2 | | 103.2 | ||
| 34.5 | | 34.5 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
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| T | | T | ||
Line 503: | Line 503: | ||
| 31.9 | | 31.9 | ||
| 80 | | 80 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
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| T | | T | ||
Line 514: | Line 514: | ||
| 12.3 | | 12.3 | ||
| 105.8 | | 105.8 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
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| T | | T | ||
Line 526: | Line 526: | ||
| 8.96 | | 8.96 | ||
| SG | | SG | ||
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| P | | P | ||
| eclipsing | | eclipsing | ||
Line 547: | Line 547: | ||
| 28.78 | | 28.78 | ||
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− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
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| T? | | T? | ||
Line 558: | Line 558: | ||
| 168.8 | | 168.8 | ||
| 24.3 | | 24.3 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
| | | | ||
| T? | | T? | ||
Line 569: | Line 569: | ||
| 93.7 | | 93.7 | ||
| 249.48 | | 249.48 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
− | | [[ | + | | [[List of cyclotron line sources|C]]? |
| T | | T | ||
| outbursts predicted precisely | | outbursts predicted precisely | ||
Line 580: | Line 580: | ||
| 862 | | 862 | ||
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− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
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| P? | | P? | ||
Line 603: | Line 603: | ||
| 2.09 | | 2.09 | ||
| SG | | SG | ||
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| P | | P | ||
| disk-fed HMXB | | disk-fed HMXB | ||
Line 613: | Line 613: | ||
| 407 | | 407 | ||
| 24? | | 24? | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| T | | T | ||
| | | | ||
Line 635: | Line 635: | ||
| 292 | | 292 | ||
| 187.5 | | 187.5 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
| | | | ||
| PT | | PT | ||
Line 646: | Line 646: | ||
| 264.52 | | 264.52 | ||
| ~146 | | ~146 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
| | | | ||
| PT | | PT | ||
Line 658: | Line 658: | ||
| 41.5 | | 41.5 | ||
| SG | | SG | ||
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| P | | P | ||
| very massive companion, strong orbital variability | | very massive companion, strong orbital variability | ||
Line 690: | Line 690: | ||
| 175 | | 175 | ||
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− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
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| T | | T | ||
Line 722: | Line 722: | ||
| 272 | | 272 | ||
| 132.2 | | 132.2 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| T | | T | ||
| Strong spectral parameter variations | | Strong spectral parameter variations | ||
Line 744: | Line 744: | ||
| 17.6 | | 17.6 | ||
| 42.12 | | 42.12 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
| | | | ||
| T | | T | ||
Line 767: | Line 767: | ||
| 0.029 | | 0.029 | ||
| WD? | | WD? | ||
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| | | | ||
| Torque reversals | | Torque reversals | ||
Line 778: | Line 778: | ||
| 3.7 | | 3.7 | ||
| SG | | SG | ||
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| P | | P | ||
| | | | ||
Line 799: | Line 799: | ||
| 15.4 | | 15.4 | ||
| 132.9 | | 132.9 | ||
− | | [[BeXRB]] | + | | [[List of Be X-ray Binaries|BeXRB]] |
− | | [[ | + | | [[List of cyclotron line sources|C]] |
| T | | T | ||
| strong flares | | strong flares | ||
Line 832: | Line 832: | ||
| 5880 | | 5880 | ||
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− | | [[ | + | | [[List of symbiotic X-ray binaries|SyXB]] |
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Line 843: | Line 843: | ||
| 912 | | 912 | ||
| 3.7 | | 3.7 | ||
− | | [[ | + | | [[List of symbiotic X-ray binaries|SyXB]] |
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Line 887: | Line 887: | ||
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Line 931: | Line 931: | ||
| 626 | | 626 | ||
| ? | | ? | ||
− | | [[ | + | | [[List of symbiotic X-ray binaries|SyXB]] |
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| | | |
Revision as of 11:31, 18 April 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.
# | 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.