Crowther, P. A. and Clark, J. S.
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We discuss evidence in favour of the Wolf-Rayet star #17-A from Massey et al. and Crowther et al. being the optical counterpart to the X-ray bright source IC10 X-1, on the basis of recent Chandra and HST/ACS imaging by Bauer & Brandt plus Gemini GMOS spectroscopy. Subject to confirmation of a short orbital period and line-profile variability, this early-type WN+cc system appears to be a counterpart to Cyg X-3 in the starburst galaxy IC10.
|Item Type:||Journal Article|
|Copyright Holders:||2007 Astronomical Society of the Pacific|
|Extra Information:||Massive Stars in Interacting Binaries
Proceedings of a workshop held at Hotel Sacacomie, Mauricie, Québec, Canada
16-20 August 2004
Edited by: Nicole St-Louis and Anthony F.J. Moffat
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Users 9108 not found.|
|Date Deposited:||09 Dec 2009 16:13|
|Last Modified:||04 Oct 2016 10:30|
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