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Confining the Edges of the GW Vir Instability Strip

Published online by Cambridge University Press:  12 April 2016

K. Werner ,
T. Rauch ,
S. Dreizler  and
U. Heber
K. Werner
Affiliation:
Institut für Astronomie und Astrophysik der Universität, Kiel, Germany
T. Rauch
Affiliation:
Institut für Astronomie und Astrophysik der Universität, Kiel, Germany
S. Dreizler
Affiliation:
Sternwarte Bamberg, Universität Erlangen-Nürnberg, Germany
U. Heber
Affiliation:
Sternwarte Bamberg, Universität Erlangen-Nürnberg, Germany

Abstract

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Ground based optical spectroscopy as well as EUVE and HST observations are used for model atmosphere analyses of PG1159 stars in order to confine the GW Vir instability strip.

Information

Type
Part 1. The Scientific Programme
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 96 - 97
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Dreizier, S., Werner, K., Heber, U. 1995, in White Dwaxfs, Lecture Notes in Physics 443, eds. Koester, D. and Werner, K., Springer, p. 160 Google Scholar
Stanghellini, L., Cox, A.N., Starrfield, S. 1991, ApJ, 383, 766 Google Scholar
Starrfield, S., Cox, A.N., Kidman, R.B., Pesnell, W.D. 1984, ApJ, 281, 800 Google Scholar