Kühnel, M. and Kretschmar, P. and Fürst, F. and Pottschmidt, K. and Hemphill, P. and Rothschild, R. E. and Okazaki, A. T. and Sagredo, M. and Wilms, J. (2017) Be-Phenomenon in Neutron Star X-ray Binaries. In: The B[e] Phenomenon: Forty Years of Studies. Astronomical Society of the Pacific Conference Series. No.508. Astronomical Society of the Pacific , San Francisco, CA, pp. 385-386. ISBN 978-1-58381-900-5. https://resolver.caltech.edu/CaltechAUTHORS:20170608-134647452
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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.
Item Type: | Book Section | ||||||||||||
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Additional Information: | © 2017 Astronomical Society of the Pacific. MK acknowledges funding by the European Space Agency under contract 4000115860/15/NL/IB. | ||||||||||||
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Series Name: | Astronomical Society of the Pacific Conference Series | ||||||||||||
Issue or Number: | 508 | ||||||||||||
Record Number: | CaltechAUTHORS:20170608-134647452 | ||||||||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20170608-134647452 | ||||||||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||||||
ID Code: | 78034 | ||||||||||||
Collection: | CaltechAUTHORS | ||||||||||||
Deposited By: | Ruth Sustaita | ||||||||||||
Deposited On: | 08 Jun 2017 21:39 | ||||||||||||
Last Modified: | 17 Dec 2019 22:25 |
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