Hostname: page-component-848d4c4894-pjpqr Total loading time: 0 Render date: 2024-06-16T04:48:46.767Z Has data issue: false hasContentIssue false
  • English
  • Français

Nuclei of Planetary Nebulae in the Pulsation Instability Strip

Published online by Cambridge University Press:  12 April 2016

W. Dziembowski
W. Dziembowski*
Affiliation:
Copernicus Astronomical Center, Polish Academy of Sciences, Aleje Ujazdowskie 4, 00-478 Warszawa, POLAND

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.

Pulsation properties of relevant stellar models are investigated with the linear nonadiabatic method. Short-period variability of FG Sge is interpreted as a pulsation phenomenon.

Type
Part II: Cataclysmic Variables
Information
International Astronomical Union Colloquium , Volume 42: The Interaction of Variable Stars with their Environment , 1977 , pp. 342 - 345
Copyright
Copyright © Veröff. Der Remeis-Sterwarte 1977

References

Acker, A. 1977, Astron. Astrophys. in pressGoogle Scholar
Christy-Sackmann, I.-J., Despain, K.H. 1974, Astrophys. J. 189, 523 Google Scholar
Langer, G.E., Kraft, R.P., Anderson, K.S. 1974, Astrophys. J. 189, 509 Google Scholar
Paczyński, B. 1970, Acta Astron. 20, 47 Google Scholar
Paczyński, B. 1974, Astrophys. J. 192, 483 Google Scholar
Paczyński, B. 1975, Astrophys. J. 202, 558 Google Scholar
Papousek, J. 1972, Scripta Fac. Sci. Nat. Ujep Brunensis. Physica 2, 2, 115Google Scholar
Smoliński, J., Clinenhaga, J.L., Kipper, T. 1976, Publ. Astr. Soc. Pac. 86, 67 Google Scholar
Sparks, W., Kutter, G. 1973, Astrophys. J. Letters 183, L121 Google Scholar
Stellingwerf, R.F. 1975, Astrophys. J. 195, 441 CrossRefGoogle Scholar