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A 10-Day Binary System Orbiting the Be Star 66 Oph

Published online by Cambridge University Press:  26 May 2016

S. Štefl ,
P. Hadrava ,
D. Baade ,
Th. Rivinius ,
M. Maintz  and
O. Stahl
S. Štefl
Affiliation:
Astronomical Institute, Academy of Sciences, CZ-251 65 Ondřejov, Czech Republic
P. Hadrava
Affiliation:
Astronomical Institute, Academy of Sciences, CZ-251 65 Ondřejov, Czech Republic
D. Baade
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching bei München, Germany
Th. Rivinius
Affiliation:
Landessternwarte Königstuhl, D-69117, Heidelberg, Germany
M. Maintz
Affiliation:
Landessternwarte Königstuhl, D-69117, Heidelberg, Germany
O. Stahl
Affiliation:
Landessternwarte Königstuhl, D-69117, Heidelberg, Germany

Abstract

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66 Oph is a multiple system with a close binary orbiting the B2Ve primary Be star. The binary parameters were derived by two independent methods and spectra of components BA and BB were separated by Fourier disentangling.

Type
Session 1 Observations of Rotating Stars
Information
Symposium - International Astronomical Union , Volume 215: Stellar Rotation , 2004 , pp. 166 - 167
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Floquet, M., Neiner, C., Janot-Pacheco, E., Hubert, A.-M., Jankov, S., Zorec, J., Briot, D., Chauville, J., Leister, N.V., Percy, J.R., Ballereau, D., Bakos, A.G. 2002, A&A 394, 137 Google Scholar
Hadrava, P. 1997, A&AS 122, 581 Google Scholar
Hadrava, P. 2002, http://www.asu.cas.cz/had/fotel.html Google Scholar