Table 4.
Parameters of HMXBs with a neutron star or black hole companion.
| Binary | Sp. Type | log(L/L⊙) | Teff (K) | R* (R⊙) | M* (M⊙) | D (R⊙) | LX (erg s−1) | Ṁ (M⊙ yr−1) | tX | Reference |
|---|---|---|---|---|---|---|---|---|---|---|
| X Pere | B0Ve | 4.69 | 32 000a | 7.2a | 15.5 | 420 | 1.2 × 1035 | 1.5 × 10−8 | 0.1 | 18, 66 |
| IGR J08408–4503e, f | O8.5I | 5.83 | 34 000 | 23.8 | 30 | 59 | 3.3 × 1032 | 1.1 × 10−6 | 2.3 | 50, 51, 52 |
| PSR B1259–63e, b | O9.5Ve | 4.9 | 34 000c | 8.1c | 10 | 1000 | 3.5 × 1034 | 3.2 × 10−8 | 0.2 | 21, 22 |
| IGR J16207–5129f | B1Ia | 5.4 | 29 000a | 20 | 20 | 40 | 2 × 1034 | 2.2 × 10−7 | 0.4 | 35, 36 |
| AX J16319–4752 | O8I | 5.63 | 33 000 | 20 | 35a | 32 | 7.8 × 1034 | 5.1 × 10−7 | 0.5 | 57, 58 |
| IGR J16328–4726f | O8Iaf | 5.68 | 33 000a | 21.3a | 34.3a | 61 | 1.4 × 1035 | 6.2 × 10−7 | 1.1 | 53, 54 |
| IGR J16418–4532f | O8.5I | 5.69 | 32 800 | 21.7 | 30 | 31.6 | 2 × 1036 | 6.4 × 10−7 | 0.6 | 9, 38 |
| IGR J16465–4507f | O9.5Ia | 5.69 | 30 000a | 26 | 28 | 124 | 6.8 × 1036 | 6.4 × 10−7 | 1.5 | 31, 32 |
| IGR J16479–4514f | O8.5Iab | 5.52 | 31 000a | 20 | 35 | 31.6 | 1.09 × 1034 | 3.4 × 10−7 | 0.3 | 11 |
| IGR J16493–4348 | B0.5Ia | 5.76 | 28 000a | 32.2 | 47 | 55 | 1.3 × 1034 | 8.2 × 10−7 | 0.6 | 64, 65 |
| 4U 1700–377e | O6.5Iaf | 5.81 | 35 000 | 22 | 46 | 35 | 2.2 × 1036 | 1.0 × 10−6 | 0.9 | 7, 8, 63 |
| IGR J17252–3616 | B0Ia | 5.79 | 30 000 | 29 | 15 | 51 | 1.6 × 1037 | 9.1 × 10−7 | 6.9 | 12, 13, 40 |
| IGR J17354–3255f | O9.5Iab | 5.56 | 30 000a | 22.4a | 28.8a | 54 | 1.8 × 1036 | 3.9 × 10−7 | 0.7 | 48, 49 |
| XTE X1739–302f | O8.5Iab | 5.65 | 32 000a | 21.7a | 32.2a | 173 | 4.8 × 1033 | 5.4 × 10−7 | 1.4 | 46, 47 |
| IGR J17544–2619f | O9Ib | 5.4 | 29 000 | 20.0 | 25.9 | 38.0 | 1.7 × 1035 | 2.2 × 10−7 | 0.3 | 33, 34, 56 |
| SAX J1818.6–1703f | B0.5Iab | 5.7 | 28 000a | 30 | 25 | 120 | 6 × 1035 | 6.5 × 10−7 | 1.5 | 61, 62 |
| LS 5039e | O6.5V | 5.19 | 37500 | 9.3 | 22.9 | 34.5 | 6 × 1034 | 9.6 × 10−8 | 0.3 | 26, 39, 44, 45, 59 |
| IGR J18450–0435f | O9Ia | 5.58 | 30 000 | 23 | 30 | 72 | 8 × 1036 | 4.3 × 10−7 | 0.8 | 16, 17, 43 |
| 4U 1907+09 | O8.5Iab | 5.68 | 29 760 | 26.2 | 26.0 | 54 | 2 × 1036 | 6.2 × 10−7 | 1.0 | 25 |
| IGR J19140+0951 | B0.5I | 5.47 | 28 000a | 23.2a | 25.4a | 70 | 3 × 1035 | 2.8 × 10−7 | 0.6 | 23 |
| Cyg X–1e | O9.7Iab | 5.57 | 32 000 | 19.9d | 24.0 | 42.4 | 1.4 × 1037 | 4.1 × 10−7 | 0.8 | 27, 28, 41 |
| 4U 2206+54 | O9.5Ve | 4.7 | 32 000a | 7.3 | 16 | 76 | 1.8 × 1035 | 1.6 × 10−8 | 0.1 | 24, 60 |
Notes.
Stellar parameters are taken from the literature, except for the mass-loss rate, for which we used fits of Krtička & Kubát (2017), and for the optical depth parameter, which was calculated from Eq. (13).
Derived using the expressions of Martins et al. (2005a).
Some alternative designations: X Per (HR 1209), IGR J08408-4503 (LM Vel, HD 74194), PSR B1259-63 (CPD-63°2495), 4U 1700-377 (V884 Sco, HD 153919), LS 5039 (V479 Sct), Cyg X-1 (V1357 Cyg, HD 226868), and 4U 2206+54 (BD+53°2790).
Supergiant fast X-ray transient (Lutovinov et al. 2013; Walter et al. 2015; Giménez-García et al. 2015).
References. (7) Clark et al. (2002), (8) van der Meer et al. (2005), (9) Drave et al. (2013), (11) Sidoli et al. (2013), (12) Mason et al. (2011), (13) Manousakis et al. (2012), (16) Goossens et al. (2013), (17) Sguera et al. (2007), (18) Tomsick & Muterspaugh (2010), (21) Sushch et al. (2013), (22) Sierpowska-Bartosik & Bednarek (2008), (23) Prat et al. (2008), (24) Ribó et al. (2006), (25) Cox et al. (2005), (26) Casares et al. (2005), (27) Herrero et al. (1995), (28) Hadrava & Čechura (2012), (31) Clark et al. (2010), (32) La Parola et al. (2010), (33) Drave et al. (2014), (34) Pellizza et al. (2006), (35) Tomsick et al. (2009), (36) Bodaghee et al. (2010), (38) Chaty et al. (2008), (39) Herrero et al. (2002), (40) Thompson et al. (2007), (41) Yan et al. (2008), (43) Zurita Heras & Walter (2009), (44) Moldón et al. (2012), (45) McSwain et al. (2004), (46) Drave et al. (2010), (47) Bodaghee et al. (2011), (48) Sguera et al. (2011), (49) Sguera (2013), (50) Götz et al. (2007), (51) Bozzo et al. (2010), (52) Gamen et al. (2015), (53) Fiocchi et al. (2013), (54) Romano et al. (2014), (56) Giménez-García et al. (2016), (57) Giménez-García et al. (2015), (58) Rahoui et al. (2008), (59) Martocchia et al. (2005), (60) Corbet et al. (2007), (61) Zurita Heras & Chaty (2009), (62) Boon et al. (2016), (63) Falanga et al. (2015), (64) Cusumano et al. (2010), (65) Romano (2015), and (66) Lutovinov et al. (2012).
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