Do the γ Cas X-rays come from the Be Star?
Abstract
We discuss the origin of the hard X-rays in γ Cas and its analogs. Of great importance are their temporal correlations with optical/UV signatures, suggesting an origin near the Be star.
- Publication:
-
Active OB Stars: Structure, Evolution, Mass Loss, and Critical Limits
- Pub Date:
- July 2011
- DOI:
- 10.1017/S1743921311011057
- Bibcode:
- 2011IAUS..272..428S
- Keywords:
-
- stars: emission-line;
- Be;
- stars: winds;
- outflows;
- stars: magnetic fields;
- X-rays: stars