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Evidence of Prominences on Cool Late-type Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
We review the observed characteristics of co-rotating clouds of neutral hydrogen recently detected in rapidly rotating, chromospherically active late-type stars and commonly termed “stellar prominences”. Their observed properties are placed in an overall interpretive framework and compared to standard solar prominences.
- Type
- Stellar Filaments
- Information
- International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 226 - 234
- Copyright
- Copyright © Astronomical Society of the Pacific 1998