Table 3.
Basic parameters of the systems and their type-II outbursts properties discussed in this paper.
| Spin | Magnetic field | Orbital | Start – End | Outburst | |||||
|---|---|---|---|---|---|---|---|---|---|
| Name | period | strength | period | Distance | Companion | Eccentricity | date | duration | Fluence |
| (s) | (1012 G) | (days) | (kpc) | type | (MJD) | (days) | (106 counts cm−2) | ||
| 4U 0115+63 | 3.62 (a) | 1.3 (b) | 24.3 (c) | 7.2 (d) | B0.2Ve (e) | 0.34 (e) | 57307–57341 | 34 | ∼0.14 |
| V 0332+53 | 4.37 (f) | 3.0 (g) | 33.9 (h) | 5.1 (d) | O8-9Ve (i) | 0.37 (h) | 57193–57307 | 114 | ∼0.83 |
| GRO J1750−27 | 4.45 (j) | 2.0–4.5 (k),(l) | 29.8 (m) | 12–22 (d),(k),(l) | B0-2Ve? (l) | 0.36 (m) | 57020–57146 | 126 | ∼0.50–1.67 |
Notes. The fluence during outburst is given as a relative value (in instrument units) and it is normalised assuming a distance of 7 kpc for each source.
References.(a)Cominsky et al. (1978); (b)Raguzova & Popov (2005); (c)Rappaport et al. (1978); (d)See Appendix A; (e)Negueruela & Okazaki (2001); (f)Stella et al. (1985); (g)Makishima et al. (1990); (h)Doroshenko et al. (2016); (i)Negueruela et al. (1999); (j)Bildsten et al. (1997); (k)Shaw et al. (2009); (l)Lutovinov et al. (2019); (m)Scott et al. (1997).
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