The formation of planetary nebulae with close binary nuclei

Details The formation of planetary nebulae with close binary nuclei The formation of planetary nebulae with close binary nuclei

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.188....1l&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 188, July, 1979, p. 1-12.

Astronomy and Astrophysics

Astronomy

68

Astronomical Models, Binary Stars, Mass Transfer, Planetary Nebulae, Companion Stars, Main Sequence Stars, Red Giant Stars, Stellar Mass Ejection

Scientific paper

A model for the formation of planetary nebulae with a close binary as a nucleus is presented. The model is based on mass loss instability at L2. The instability is demonstrated. The conditions on the mass loss are formulated and analysed. The observational consequence of the model is described briefly and its relation to symbiotic stars and cataclysmic binaries discussed.

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