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On the lambda-parameter of the common envelope evolution

Abstract:
The binding energy of the envelope to the core of a donor star will determine the outcome of a binary evolving through a common envelope (CE) and spiral-in phase. This binding energy is expressed by a parameter lambda which depends strongly on the evolutionary stage (i.e. stellar radius). Following our earlier publication, we present the lambda-parameter of stars with masses 11 - 100 M..
Publication status:
Published

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Volume:
229
Pages:
255-259
Publication date:
2001-01-01
URN:
uuid:7b437566-4573-44fc-8a26-54e7debb5307
Source identifiers:
10435
Local pid:
pubs:10435
ISBN:
1-58381-061-7
Keywords:

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