Pulsation of high luminosity helium stars

Author
Abstract

A discussion of the long period R Coronae Borealis stars is presented. The constraints on theoretical models imposed by their age, kinematics and distribution led to difficulties in formulating an evolutionary sequence to the formation of this type of star. Several types of models are investigated and the results given.

Year of Conference
1980
Start Page or Article ID
161-168
Publisher
Springer Berlin Heidelberg
Conference Location
Berlin, Heidelberg
ISBN Number
978-3-540-39297-2
DOI
10.1007/3-540-09994-8_14
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Publication Status
JILA PI
JILA Topics
Conference Proceedings