Author:
Hirata Ryuko,Okazaki Atsuo T.
Abstract
AbstractWe 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.
Publisher
Cambridge University Press (CUP)
Cited by
2 articles.
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1. Non-LTE Calculation for the Be Star Decretion Disk;Publications of the Astronomical Society of Japan;2008-08-25
2. Forty Years of Spectroscopic Stellar Astrophysics in Japan;Publications of the Astronomical Society of Japan;2005-02-25