Planetary nebulae in planetary and binary systems

descriptionPublicationkeyboard_double_arrow_right Article 01 Jul 1981 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 77, pages 319-324 (issn: 0004-640X, eissn: 1572-946X,

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Authors: Kyu H. Choi; Samuel C. Vila;

doi: 10.1007/bf00649462

Planetary nebulae in planetary and binary systems

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Abstract

The problem of the survival of a low-mass secondary orbiting a primary that becomes a planetary nebula is studied. The values of the mass of the primary are 1.0, 1.5, and 2.0M ⊙; the values of the mass of the secondary 0.001M ⊙, 0.01M ⊙ and 0.1M ⊡. The orbital decay and mass of the secondary due to accretion and gravitational drag in the common envelope are presented. The possible application of the results to V471 Tau, UU Sge, WZ Sge and the Sun-Jupiter system are discussed.

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University of Pennsylvania
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