Table 8
Esimates of a BH mass and a distance value for the target sources, Swift J1644+57 and Swift J2058+05, and those for reference sources.
| Source |  (M⊙) |
iorb† (deg) | d†† (kpc) | Mfund.plane (M⊙) | Mmin.timescale (M⊙) | Mscal (M⊙) |
|
|
||||||
| GX 339-4(1,2) | >6c(1) | ... | 7.5 ± 1.6(2) | ... | ... | 5.7 ± 0.8††† |
| 4U 1543-47(3,4) | 9.4 ± 1.0 | 20.7 ± 1.5 | 7.5 ± 1.0 | ... | ... | 9.4 ± 1.4††† |
| Cyg X–1(5) | 6.8–13.3 | 35 ± 5 | 2.5 ± 0.3 | ... | ... | 7.9 ± 1.0††† |
| GRO J1655–40 | 6.3 ± 0.3(7,8) | 70 ± 1(7,8) | 3.2 ± 0.2(9) | ... | ... | ... |
| Swift J1644+57(10,11,12,13,14) | ... | ... | ~ 1.5 × 106 | ~ 3 × 106 | ~ 107−109 | ≥ 7.8 × 106 |
| Swift J2058+05(14,15,16) | ... | ... | ~ 3.7 × 106 | ... | ~ 5 × 107 | ≥ 2 × 107 |
Notes.
Source distance found in the literature. For Swift J2058+0516 the distance is estimated using the redshift z with taking into account the cosmological effects for z> 1 (see Wright 20067 ).
Reference. (1) Munoz-Darias et al. (2008); (2) Hynes et al. (2004); (3) Orosz (2003); (4) Park et al. (2004); (5) Herrero et al. (1995); (6) Ninkov et al. (1998); (7) Green et al. (2001); (8) Hjellming & Rupen (1995); (9) Jonker & Nelemans (2004); (10) Miller & Gultekin (2011); (11) Bloom et al. (2011); (12) Burrows et al. (2011); (13) Levan et al. (2011); (14) Komossa (2015); (15) Cenko et al. (2012); (16) Pasham et al. (2015).
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