Table 4
Main results for the probably X-ray binary identified in the present sample of 2PBC sources.
| Object | Hα | Hβ | R | A V | d | Spectral | L X | ||
|
|
|||||||||
| EW | Flux | EW | Flux | mag | (mag) | (kpc) | type | ||
|
|
|||||||||
| 2PBC J1911.4+1412 | 12.3 ± 0.6 | 1.5 ± 0.1 | 6.3 ± 1.5 | 0.4 ± 0.1 | 17.5 | ~0.85 | ~21 | late spectral type | 7.4 (15–150)C |
| 1.4 (0.3–10)X | |||||||||
Notes. Equivalent widths (EWs) are expressed in Å, line fluxes are in units of 10-15 erg cm-2 s-1 and distance was calculated assuming MV~ 0 mag. 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).
From Cusumano et al. (2010).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.