X-ray and gamma-ray emission from single and binary early-type stars

Details X-ray and gamma-ray emission from single and binary early-type stars X-ray and gamma-ray emission from single and binary early-type stars

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005mshe.work....3s&link_type=abstract

"Proceedings of "Massive Stars and High-Energy Emission in OB Associations", a workshop of the JENAM 2005, "Distant Worlds", hel

Physics

1

Scientific paper

Since their launch, both the Chandra and XMM-Newton satellites have provided us with a new and more detailed view of the high energy processes in massive stars. This paper reviews recent X-ray observations of a range of massive stars, both O-stars and Wolf-Rayet (W-R) stars, as well as both single early-type stars and binary systems, where colliding winds may well play a role. Results from high spectral resolution X-ray data will be reviewed, where the velocity structure of the individual line profiles can be resolved. Recent INTEGRAL gamma-ray observations of massive stars will be covered, as well as discussing the expected gamma-ray properties of early-type stars.

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