Near-infrared survey of high mass X-ray binary candidates

J. M. Torrejón; I. Negueruela; D. M. Smith; T. E. Harrison

doi:10.1051/0004-6361/200912619

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Volume 510 (February 2010)

A&A, 510 (2010) A61

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Table 3:

Derived parameters for stars in our sample, calculated using the observed data.
Source	Spectral type	Class	E(B-V)	E(J-K)	M_V	M_K	d (kpc)	$L_{\rm X}$ (erg/s)^a
IGR J18027-2016	B1 Ib	SGXB	$3.04\pm0.02$	1.54	-5.8	-5.1	$12.4\pm 0.1$	( $1.65\pm0.03)\times 10^{36}$
SAX J18186-1703	B0.5 Iab	SFXT	$5.08\pm0.05$	2.54	-6.4	-5.65	$2.1\pm0.1$	( $8\pm0.4$ ) $\times 10^{35}$
IGR J18483-0311	B0-1 Iab	SFXT	$5.22\pm0.02$	2.61	-6.4	-5.66	$2.83\pm 0.05$	( $1.9\pm0.06$ ) $\times 10^{36}$
IGR J19140+0951	B0.5 Iab-a	SGXB	$5.5\pm0.1$	2.75	$-6.65\pm 0.03$	$-5.90\pm0.25$	$3.6\pm 0.04$	( $1.6\pm0.3$ ) $\times 10^{36}$
XTE 1901+014	G5 III - A3 V	LMXB?	$\sim$ 3.7	1.8			2-7	1 $^{+1}_{-0.8}\times 10^{38}$

Notes. ^(a) Opeak luminositites for the energy ranges (2-10) keV, (22-55) keV, (20-100) keV, (2-20) keV and (3-12) keV respectively.

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