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Crowther, P. A. and Clark, J. S.
(2007).
URL: http://www.aspbooks.org/a/volumes/article_details/...
Abstract
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.
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- Item ORO ID
- 19119
- Item Type
- Journal Item
- Extra Information
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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
ISBN: 978-1-583812-35-8 - Academic Unit or School
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Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Copyright Holders
- © 2007 Astronomical Society of the Pacific
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