Table 1
Optical and X-ray information of the systems and the outbursts analysed in this work.
| Source | Spectral | P spin | P orb | e | E cyc | QPO | Distance | Outburst |
|
/LEdd |
/Lcrit |
References |
| name | type | (s) | (days) | (keV) | (mHz) | (kpc) | duration (d) | (erg s-1) | ||||
|
|
||||||||||||
| V 0332+53 | O8-9V | 4.4 | 34.2 | 0.42 | 25 | 51, 223 | 7 | 100 | 3.4 × 1038 | 2.0 | 10 | 1, 2, 3 |
| EXO 2030+375 | B0.5III-V | 41.8 | 46.0 | 0.41 | 11 | 200 | 7.1 | 155 | 1.6 × 1038 | 0.9 | 11 | 4, 5, 6 |
| 4U 0115+63 | B0.2V | 3.6 | 24.3 | 0.34 | 12 | 2, 62 | 8.1 | 55 | 1.4 × 1038 | 0.8 | 9 | 7, 8, 9 |
| KS 1947+300 | B0V | 18.7 | 40.4 | 0.03 | – | 20 | 10 | 165 | 7.1 × 1037 | 0.4 | ~7† | 10, 11 |
| 1A 0535+262 | B0III | 105 | 111 | 0.47 | 46 | 27–72 | 2.4 | 45 | 6.8 × 1037 | 0.4 | ≲1 | 12, 13, 14 |
| Swift J1626.6–5156 | B0V | 15.4 | 133 | 0.08 | – | – | ~10 | ~100 | 5.2 × 1037 | 0.3 | – | 15, 16, 17 |
| XTE J0658–073 | O9.7V | 160.7 | 101 | – | 33 | – | 3.9 | 105 | 3.6 × 1037 | 0.2 | ≲1 | 18, 19, 20 |
| 1A 1118–616 | O9.5III-V | 405 | 24 | 0.0 | 60 | 80 | 5 | 30 | 2.9 × 1037 | 0.2 | 0.4 | 21, 22, 23, 24 |
| GRO J1008–57 | B1-B2III-V | 93.5 | 247.8 | 0.68 | – | – | 5 | 50 | 2.0 × 1037 | 0.1 | – | 25, 26, 27 |
Notes. The X-ray luminosity quoted is for the 3–30 keV energy range. The critical luminosity depends on the energy of the cyclotron line (see Becker et al. 2012, and Sect. 5.2). A “–” sign indicates that either the parameter has not been detected or it is not known. †: Estimated from the break observed in the Γ−Lx diagram, and not from Ecyc (see Sect. 5.2).
References. [1] Raichur & Paul (2010); [2] Negueruela et al. (1999); [3] Qu et al. (2005); [4] Angelini et al. (1989); [5] Wilson et al. (2002); [6] Wilson et al. (2008); [7] Li et al. (2012); [8] Reig et al. (2007); [9] Heindl et al. (1999); [10] Negueruela et al. (2003); [11] Galloway et al. (2004); [12] Caballero et al. (2007); [13] Clark et al. (1998); [14] Finger et al. (1996); [15] Baykal et al. (2010); [16] Reig et al. (2011); [17] Içdem et al. (2011); [18] McBride at al. (2006); [19] Yan et al. (2012); [20] Nespoli et al. (2012); [21] Coe et al. (1994a); [22] Doroshenko et al. (2010); [23] Staubert et al. (2011); [24] Nespoli & Reig (2011); [25] Coe et al. (1994b); [26] Shrader et al. (1999); [27] Naik et al. (2011).
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