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Evidence of Prominences on Cool Late-type Stars

Published online by Cambridge University Press:  12 April 2016

P.B. Byrne ,
M.T. Eibe  and
G.H.J. van den Oord
P.B. Byrne
Affiliation:
Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland
M.T. Eibe
Affiliation:
Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland
G.H.J. van den Oord
Affiliation:
Sterrekundig Instituut, Postbus 80.000, 3508 TA Utrecht, The Netherlands

Abstract

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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.

Information

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

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