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Table 3.

Derived tangential peculiar velocities and orbital eccentricity values compiled from the literature.

Name vpec, BJ vpec, iso e e ref
(km s−1) (km s−1)
4U 0115+63 0.342 ± 0.004 Raichur & Paul (2010)
V 0332+53 0.417 ± 0.007 Raichur & Paul (2010)
GS 0834-430 0.14 ± 0.04 Wilson et al. (1997)
IGR J19294+1816
XTE J1946+274 0.33 ± 0.05 Wilson et al. (2003)
4U 1416-62 0.417 ± 0.003 Raichur & Paul (2010)
KS 1947+300 0.033 ± 0.013 Galloway et al. (2004)
GS 1843+00
RX J0812.4-3114
EXO 2030+375 0.412 ± 0.001 Wilson et al. (2008)
IGR J22534+6243
AX J1700.2-4220
Cep X-4
XTE J1906+090 0.03 <  e <  0.06 Wilson et al. (2002)
GRO J1008-57 0.68 ± 0.02 Coe et al. (2007)
3A 0535+262 0.47 ± 0.02 Finger et al. (1994)
4U 0728-25
2E 0655.8-0708 e ∼ 0.4 Yan et al. (2012)
IGR J11435-6109
GRO J2058+42
RX J0440.9+4431 e >  0.4 Yan et al. (2016)
GX 304-1 e ∼ 0.5 Sugizaki et al. (2015)
4U 1145-619 e ∼ 0.8 Watson et al. (1981)
SAX J2103.5+4545 0.406 ± 0.004 Baykal et al. (2007)
1A 1118-615 0 <  e <  0.16 Staubert et al. (2011)
IGR J01583+6713
2RXP J130159.6-635806
4U 0352+309 0.111 ± 0.018 Delgado-Martí et al. (2001)
3U 1022-55
SAX J2239.3+6116
RX J0146.9+6121
4U 2206+543 e ∼ 0.15 Ribó et al. (2006)
1H 1249-637

Notes. vpec, BJ denotes the velocities obtained using the priors adopted from Bailer-Jones et al. (2018), and vpec, iso are the velocities obtained using the empirically determined scale length derived in Sect. 2.2.

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