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The Line Profile Variations of 60 Cyg (HD 200310)*

Published online by Cambridge University Press:  12 April 2016

P. Koubský ,
D. Ballereau ,
J. Chauville  and
J. Horn
P. Koubský
Affiliation:
Astronomical Institute, Academy of Sciences of Czech Republic, CZ-251 65 Ondřejov, Czech Republic
D. Ballereau
Affiliation:
Observatoire de Paris, Section d’Astrophysique de Meudon, F-92195 Meudon Principal Cedex, France
J. Chauville
Affiliation:
Observatoire de Paris, Section d’Astrophysique de Meudon, F-92195 Meudon Principal Cedex, France
J. Horn
Affiliation:
Astronomical Institute, Academy of Sciences of Czech Republic, CZ-251 65 Ondřejov, Czech Republic

Abstract

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Results of the preliminary investigation of the monitoring of line-profile variations of the Be star 60 Cyg are reported. At least three apparent absorption or emission bumps moving from blue to red were detected.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 307 - 308
Copyright
Copyright © Astronomical Society of the Pacific 1995

Footnotes

†

Jiři Horn died December 13, 1994

*

Based on observations collected at the Haute Provence Observatory

References

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