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: | 03 Oct 2019 18:04 |
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