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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

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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