Crowther, P. A. and Clark, J. S.
(2007).
| URL: | http://www.aspbooks.org/a/volumes/article_details/... |
|---|---|
| Google Scholar: | Look up in Google Scholar |
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.
| Item Type: | 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 ISBN: 978-1-583812-35-8 |
| Academic Unit/School: | 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) |
| Related URLs: | |
| Item ID: | 19119 |
| Depositing User: | Users 9108 not found. |
| Date Deposited: | 09 Dec 2009 16:13 |
| Last Modified: | 04 Oct 2016 10:30 |
| URI: | http://oro.open.ac.uk/id/eprint/19119 |
| Share this page: |     |