Ephemeris, orbital decay, and masses of ten eclipsing high-mass X-ray binaries

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Volume 577 (May 2015)

A&A, 577 (2015) A130

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Table 9

Properties of the stellar winds in the ten HMXBs as inferred from observations and theoretical calculations.

Source	v_∞	v_∞	Ṁ
	km s^-1	km s^-1	M_⊙ yr^-1
	observed	theoretical	theoretical

LMC X-4	1350(35)^a	1950(600)	2.4 × 10^-7
Cen X-3	~500^b	2050(600)	5.3 × 10^-7
4U 1700-377	1700(100)^c	1850(550)	> 2.1 × 10^-6
4U 1538-522	− ^d	1000(300)	8.3 × 10^-7
SMC X-1	− ^d	870(260)	1.5 × 10^-6
SAX J1802.7-2017	− ^d	680(200)	6.3 × 10^-7
XTE J1855-026	− ^d	620(190)	< (0.2−1.1) × 10^-5
Vela X-1	600(100)^c	640(190)	< (1.0−5.3) × 10^-6
EXO J1722-363	− ^d	650(200)	9.0 × 10^-7
OAO 1657-415	~250^e	200(60)	< (1.1−5.6) × 10^-7

Reference.

^(a)

Boroson et al. (1999);

^(b)

Wojdowski et al. (2003);

^(c)

van Loon et al. (2001);

^(d)

No consolidated measurement available in the literature to the best of our knowledge;

^(e)

Mason et al. (2012).

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