No CrossRef data available.
Article contents
FUSE observations of the SMC Wolf-Rayet binary Sand 1 (WO4+O4V): atmospheric eclipses and colliding winds
Published online by Cambridge University Press: 26 May 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
We present FUSE observations of the SMC WO4+O4V binary Sand 1. Our spectra show variations in S iv, C iii, C iv and O vi lines, which we attribute mainly to emission from the shock cone, resulting from the collision between the two winds, and to atmospheric eclipses of the O-star continuum light by the WR wind. From this variability, we deduce a cone opening angle of 120°.
- Type
- Part 1. Atmospheres of Massive Stars
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2003
References
You have
Access