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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) MV MK 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.


Source LaTeX | All tables | In the text

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