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Puzzling X-rays from the new colliding wind binary WR 65 (WC9d)

By L. M. Oskinova and W. -r. Hamann

Abstract

More than 54 % of all Wolf-Rayet (WR) stars are in binary systems that consist of a WR and an OB-type star (Wallace 2007). The collision between two stellar winds in these systems produces characteristic signatures in different wavelength bands that can includ

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