On the lambda-parameter of the common envelope evolution

Dewi, JDM; Tauris, TM

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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APA Style

Dewi, J. D. M., & Tauris, T. M. (2001). On the lambda-parameter of the common envelope evolution. 229, 255–259.

MLA Style

Dewi, J. DM, and T. M. Tauris. On the Lambda-Parameter of the Common Envelope Evolution. 2001, pp. 255–59.

Chicago Style

Dewi, JDM, and TM Tauris. 2001. “On the Lambda-Parameter of the Common Envelope Evolution.” In , 229:255–59.
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