Hostname: page-component-7bb8b95d7b-dvmhs Total loading time: 0 Render date: 2024-10-03T04:32:59.572Z Has data issue: false hasContentIssue false
  • English
  • Français

Physics of the phase changes of Be stars

Published online by Cambridge University Press:  26 May 2016

K.K. Ghosh
K.K. Ghosh*
Affiliation:
Indian Institute of Astrophysics, Vainu Bappu Observatory, Kavalur, India

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Based on spectroscopic observations of more than 100 Be stars, we present the results of the phase changes of Be stars.

Type
6. Be Stars: Circumstellar Environment
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 351 - 353
Copyright
Copyright © Kluwer 1994 

References

Baade, D.: 1989, Astronomy and Astrophysics 198, 211 Google Scholar
Ghosh, K.K.: 1990, Astrophysical Journal 360, 239 CrossRefGoogle Scholar
Ghosh, K.K. et al., 1993, in preparation Google Scholar
Kogure, T.: 1990, Astrophysics and Space Science 193, 7 CrossRefGoogle Scholar
Peters, G.J.: 1991, Be Star News Lett. 24, 17 Google Scholar