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Emission Line Profiles from BeXRBs

Published online by Cambridge University Press:  12 April 2016

R.W. Hanuschik ,
M. Maisack ,
H. Cao  and
W. Hummel
R.W. Hanuschik*
Affiliation:
Astronomisches Institut, Ruhr-Universität, D-44780 Bochum, Germany
M. Maisack
Affiliation:
IAA, Universität Tübingen, D-72076 Tübingen, Germany
H. Cao
Affiliation:
Beijing Astronomical Observatory, Beijing 1000 080, P.R. China
W. Hummel
Affiliation:
Universitätssternwarte, Scheinerstr. 1, D-81679 München, Germany
*
1 Email address:rwh@astro.ruhr-uni-bochum.de

Abstract

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We have measured optical spectra of several BeXRBs. Their Be disks apparently do not differ significantly from those in single Be’s.

Information

Type
Part 15. Poster Papers
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 713 - 714
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Hanuschik, R.W. et al. 1995, A&A, 300, 163 Google Scholar
Hanuschik, R.W. et al. 1996, A&AS, 116, 309 Google Scholar
Waters, L.B. 1989, in Proc. 23rd ESLAB Symp., ESA SP-296, p. 25 Google Scholar