Published 2017
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Be-Phenomenon in Neutron Star X-ray Binaries
Abstract
In this work we provide a brief insight into two aspects of Be/X-ray binaries, which are probably involved in production of X-ray outbursts: the evolution of the Be star disk, in particular of its size, and the binary geometry which drives gravitational interaction. Simultaneous X-ray and optical data will aid our investigation of the evolution of Be stars in binaries and the X-ray outburst mechanism.
Additional Information
© 2017 Astronomical Society of the Pacific. MK acknowledges funding by the European Space Agency under contract 4000115860/15/NL/IB.Attached Files
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Additional details
- Eprint ID
- 78034
- Resolver ID
- CaltechAUTHORS:20170608-134647452
- 4000115860/15/NL/IB
- European Space Agency (ESA)
- Created
-
2017-06-08Created from EPrint's datestamp field
- Updated
-
2019-12-17Created from EPrint's last_modified field
- Series Name
- Astronomical Society of the Pacific Conference Series
- Series Volume or Issue Number
- 508