X-Ray Emission From Hybrid Stars
Abstract
Hybrid stars are giant stars that exhibit both chromospheric emission features and signatures of mass outflow, and hence provide a link between stars on either side of the ``Coronal Dividing Line". We have obtained long duration ROSAT PSPC exposures of two nearby hybrid stars (alpha TrA and iota Aur), and here, we compare these observations with models of X-ray emission on giant stars.
- Publication:
-
American Astronomical Society Meeting Abstracts #182
- Pub Date:
- May 1993
- Bibcode:
- 1993AAS...182.2206K