Hostname: page-component-7479d7b7d-k7p5g Total loading time: 0 Render date: 2024-07-11T08:32:11.776Z Has data issue: false hasContentIssue false
  • English
  • Français

Chemical Composition and Distribution of White Dwarfs

Published online by Cambridge University Press:  14 August 2015

Volker Weidemann
Volker Weidemann*
Affiliation:
Universität Kiel, Germany

Extract

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.

This contribution makes a few points which are relevant to the question of the fraction of white dwarfs formed via the planetary-nebula phenomenon.

Type
Session VI – Origin and Evolution
Information
Symposium - International Astronomical Union , Volume 34: Planetary Nebulae , 1968 , pp. 423 - 424
Copyright
Copyright © Reidel 1968 

References

Eggen, O.J., Greenstein, J.L. (1965) Astrophys. J., 141, 83.CrossRefGoogle Scholar
Eggen, O.J., Sandage, A.R. (1967) Astrophys. J., 148, 911.Google Scholar
Kippenhahn, R., Kohl, K., Weigert, A. (1967) Z. Astrophys., 66, 58.Google Scholar
Mestel, L., Ruderman, M.A. (1967) Mon. Not. R. Astr. Soc., 136, 27.CrossRefGoogle Scholar
Weidemann, V. (1967) Z. Astrophys., 67, 286.Google Scholar