Theory of ring formation around Be stars
Journal Article
·
· Publ. Astron. Soc. Pac.; (United States)
A quantitative theory has been developed for the formation of the gaseous rings around Be stars based on the ideas, first discussed by Gerasimovic, later developed by Huang, and independently suggested by Massa. The theory has been derived from the laws of conservation of energy and angular momentum without any other assumptions.
- Research Organization:
- Northwestern Univ., Evanston, IL
- OSTI ID:
- 7342652
- Journal Information:
- Publ. Astron. Soc. Pac.; (United States), Journal Name: Publ. Astron. Soc. Pac.; (United States) Vol. 88:524; ISSN PASPA
- Country of Publication:
- United States
- Language:
- English
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