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Interpretation of the Cyclic Balmer Progression Phenomenon

Published online by Cambridge University Press:  12 April 2016

Ryuko Hirata  and
Atsuo T. Okazaki
Ryuko Hirata
Affiliation:
Department of Astronomy, Kyoto University, Kyoto 606-8502, Japan
Atsuo T. Okazaki
Affiliation:
Faculty of Engineering, Hokkai-Gakuen University, Toyohira-ku, Sapporo 062-8605, Japan

Abstract

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We have computed the Balmer-line profiles for the one-armed oscillation model and found that the model can naturally account for the cyclic Balmer progression phenomenon observed in the V/R variable shell stars.

Type
6. Disks
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 531 - 534
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

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