XMM-Newton Observations Reveal Very High X-ray Luminosity from the Carbon-rich Wolf-Rayet Star WR 48aReport as inadecuate



 XMM-Newton Observations Reveal Very High X-ray Luminosity from the Carbon-rich Wolf-Rayet Star WR 48a


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We present XMM-Newton observations of the dusty Wolf-Rayet star WR 48a. This is the first detection of this object in X-rays. The XMM-Newton EPIC spectra are heavily absorbed and the presence of numerous strong emission lines indicates a thermal origin of the WR 48a X-ray emission, with dominant temperature components at kT cool approx. 1 keV and kT hot approx. 3~keV, the hotter component dominating the observed flux. No significant X-ray variability was detected on time scales 1 day. Although the distance to WR 48a is uncertain, if it is physically associated with the open clusters Danks 1 and 2 at d ~ 4 kpc, then the resultant X-ray luminosity L X ~ 10^35 ergs-s makes it the most X-ray luminous Wolf-Rayet star in the Galaxy detected so far, after the black-hole candidate Cyg X-3. We assume the following scenarios as the most likely explanation for the X-ray properties of WR 48a: 1 colliding stellar winds in a wide WR+O binary system, or in a hierarchical triple system with non-degenerate stellar components; 2 accretion shocks from the WR 48a wind onto a close companion possibly a neutron star. More specific information about WR48a and its wind properties will be needed to distinguish between the above possibilities.



Author: Svetozar A. Zhekov; Marc Gagne; Stephen L. Skinner

Source: https://archive.org/







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