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Table 4.
Inferred birthplace of HMXBs observed by Gaia and corresponding age since the first supernova event.
| HMXB | Birthplace | tSN | vpec | ||
|---|---|---|---|---|---|
| [Myr] |
[km s−1] |
||||
| This work | CC13 | This work | F22 | ||
| IGR J00370+6122 | Isolated | ... |
 |
||
| 1A 0114+650 | Cluster | 4.4 |
37 |
 |
|
| LS I+61 303 | Cluster | 15 – 16 | 12 – 18 |
 |
|
| X Per | Cluster | 24 |
33 |
 |
|
| XTE J0421+560 | ...( * ) | ... |
 |
||
| 1A 0535+262 | Arm | 18 |
80 | 49.7 |
 |
| IGR J06074+2205 | ...( * ) | ... | |||
| HD 259440 | Cluster | 38 |
31 |
 |
|
| IGR J08408−4503 | Isolated | ... |
 |
||
| Vela X-1 | Isolated | ... |
 |
||
| 2FGL J1019.0-5856 | Arm( * ) | 10 |
42 |
 |
|
| Cen X-3 | Arm( * ) | 1.9 |
78 |
||
| 1E 1145.1-6141 | Arm( * ) | 15 – 35 | 77 – 81 |
 |
|
| GX 301-2 | Isolated( * ) | ... |
 |
||
| PSR B1259-93 | Isolated | ... | 60 |
 |
|
| 4U 1538-522 | Arm( * ) | 4.4 – 15 | 20 | 80 – 90 |
 |
| 4U 1700-377 | Cluster | 1.9 |
80 | 110 |
 |
| IGR J17544−2619 | Cluster | 5.4 |
37 |
 |
|
| SAX J1802.7-2017 | ...( * ) | ... | |||
| LS 5039 | Isolated | ... |
 |
||
| IGR J18410−0535 | ...( * ) | ... | 60 | ||
| IGR J18450−0435 | Arm( * ) | 17 – 23 | 59 – 62 | ||
| SS 433 | Arm( * ) | < 60 | 32 |
||
| Cyg X-1 | Cluster | 4.4 |
26 |
||
| 4U 2206+543 | Arm | 21 – 32 | 38.3 |
 |
|
| MWC 656 | Isolated | ... | |||
Notes. ( * )Caveat for binaries located in regions with low cluster density (< 10 kpc−2). CC13: Coleiro & Chaty (2013), F22: Fortin et al. (2022).
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