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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
*
1Email 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.

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