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Evolutionary Status and Origin of Extremely Hydrogen-Deficient Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
Our present knowledge about the evolutionary status of extremely hydrogen-deficient stars is reviewed. Possible schemes for their creation are discussed, with special emphasis on a recently proposed binary scenario, according to which they are the result of the merging of two white dwarfs. Finally, the possible generic links between the different groups of extremely hydrogen-deficient stars are briefly discussed.
- Type
- IX Theory
- Information
- International Astronomical Union Colloquium , Volume 87: Hydrogen Deficient Stars and Related Objects , 1985 , pp. 471 - 482
- Copyright
- Copyright © Reidel 1986
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