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Be-Phenomenon in Neutron Star X-ray Binaries

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.

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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
Related URLs:
URLURL TypeDescription
Kretschmar, P.0000-0001-9840-2048
Fürst, F.0000-0003-0388-0560
Pottschmidt, K.0000-0002-4656-6881
Hemphill, P.0000-0002-1676-6954
Wilms, J.0000-0003-2065-5410
Additional Information:© 2017 Astronomical Society of the Pacific. MK acknowledges funding by the European Space Agency under contract 4000115860/15/NL/IB.
Funding AgencyGrant Number
European Space Agency (ESA)4000115860/15/NL/IB
Series Name:Astronomical Society of the Pacific Conference Series
Issue or Number:508
Record Number:CaltechAUTHORS:20170608-134647452
Persistent URL:
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:78034
Deposited By: Ruth Sustaita
Deposited On:08 Jun 2017 21:39
Last Modified:17 Dec 2019 22:25

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