The period distribution of binary systems which are predecessors of planetary nebulae

Details The period distribution of binary systems which are predecessors of planetary nebulae The period distribution of binary systems which are predecessors of planetary nebulae

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...67k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Nov.-Dec. 1986, p. 67-76. In Russian.

Physics

Binary Stars, Planetary Nebulae, Stellar Envelopes, Stellar Evolution, Stellar Orbits, Ellipticity, Mass Ratios, Stellar Mass Ejection

Scientific paper

Consideration is given to the possibility that the shape of a planetary nebula can provide information on the parameters of the binary system in which it was formed. It is shown that the observed distribution of planetary nebula shapes over ellipticities can be explained only if the nebulae did originate in the binary systems. The mass ratio distribution of the binary systems has only a small effect on the observed ellipticity function of the planetary nebulae. The period distribution law of binary systems is derived and discussed.

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