Table 7
Main results for the HMXB IGR J19173+0747 (see Fig. 7, lower right panel) identified in the present sample of INTEGRAL sources.
| Object | Hα | Hβ | He ii λ4686 | R | AV | d | Spectral | LX | |||
|
|
|||||||||||
| EW | Flux | EW | Flux | EW | Flux | mag | (mag) | (kpc) | type | ||
|
|
|||||||||||
| IGR J19173+0747 | 6.1 ± 0.6 | 1.77 ± 0.18 | <10 | <0.8 | <10 | <0.8 | 16.0 | ~4.2 | ~10 | early B V | 0.027 (0.1–2.4; R) |
| 0.72 (0.5–10; X) | |||||||||||
| 0.67 (20–40; I) | |||||||||||
Notes. EWs are expressed in Å, line fluxes are in units of 10-15 erg cm-2 s-1, whereas X-ray luminosities are in units of 1035 erg s-1 and the reference band (between round brackets) is expressed in keV. In the last column, the upper-case letter indicates the satellite and/or the instrument with which the corresponding X-ray flux measurement was obtained (see text).
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