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arXiv · 1205.3510

An X-ray Survey of Colliding Wind Binaries

Marc Gagne·Garrett Fehon·Michael Savoy·Carlos Cartagena·David H. Cohen·Stanley P. Owocki
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Abstract

We have compiled a list of 36 O+O and 89 Wolf-Rayet binary candidates in the Milky Way and Magellanic clouds detected with the Chandra, XMM-Newton and ROSAT satellites to probe the connection between their X-ray properties and their system characteristics. Of the WR binaries with published parameters, all but two have kT > 0.9 keV. The most X-ray luminous WR binaries are typically very long period systems. The WR binaries show a nearly four-order of magnitude spread in X-ray luminosity, even among among systems with very similar WR primaries. Among the O+O binaries, short-period systems generally have soft X-ray spectra and longer period systems show harder X-ray spectra, again with a large spread in LX/Lbol.

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Marc Gagne, Garrett Fehon, Michael Savoy, Carlos Cartagena, David H. Cohen, Stanley P. Owocki. 2012-05-15. An X-ray Survey of Colliding Wind Binaries. https://arxiv.org/abs/1205.3510

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