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- W2997672204 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." @default.
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- W2997672204 date "2012-12-01" @default.
- W2997672204 modified "2023-09-27" @default.
- W2997672204 title "An X-Ray Survey of Colliding Wind Binaries" @default.
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