No CrossRef data available.
Article contents
The ROSAT view of the massive eclipsing O-type binary system 29 UW Canis Majoris
Published online by Cambridge University Press: 07 August 2017
Abstract
We have investigated a recently obtained ROSAT X-ray observation of the massive binary 29 UW Canis Majoris (HR 2781; HD 57060). This short-period binary (4.3934 d) consists of two eclipsing O-type stars and has been observed for about 9 days with the ROSAT PSPC. We discuss the origin of the X-ray emission in the close binary system 29 CMa in the context of the traditional colliding wind scenario as well as the scenario of X-ray emission from shock heated gas in the stellar winds.
- Type
- Session VII - Hydrodynamics and high-energy physics of colliding winds
- Information
- Copyright
- Copyright © Kluwer 1995