Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-29T10:43:07.622Z Has data issue: false hasContentIssue false
  • English
  • Français

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 AstronomieundAstrophysik der Universität, Kiel, Germany
T. Rauch
Affiliation:
Institut für AstronomieundAstrophysik der Universität, Kiel, Germany
S. Dreizler
Affiliation:
Sternwarte Bamberg, Universität Erlangen-Nürnberg, Germany
U. Heber
Affiliation:
Sternwarte Bamberg, Universität Erlangen-Nürnberg, Germany

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

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