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Stellar Pulsation: (II) Multiple Distinct Shells

Published online by Cambridge University Press:  12 April 2016

Yu Zhi-Yao
Yu Zhi-Yao*
Affiliation:
Shanghai Observatory, 80 Nandan Road, Shanghai 200030, China

Abstract

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We can find the conclusion with our analysis for VLA observation of OH maser and CO (2–1) emission line that they are distributed on some different distinct shells in the circumstellar envelope, respectively.

Type
II. Observational Facts
Information
International Astronomical Union Colloquium , Volume 134: Nonlinear Phenomena in Stellar Variability , 1993 , pp. 169 - 172
Copyright
Copyright © Kluwer 1993

References

Bowers, P.F. et al.: 1983, Astrophysical Journal 274, 733.Google Scholar
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