Planetary nebulae in planetary and binary systems

Details Planetary nebulae in planetary and binary systems Planetary nebulae in planetary and binary systems

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..77..319c&link_type=abstract

Astrophysics and Space Science, vol. 77, no. 2, July 1981, p. 319-324.

Astronomy and Astrophysics

Astrophysics

5

Binary Stars, Planetary Nebulae, Stellar Envelopes, Stellar Mass Accretion, Orbital Mechanics, Solar Orbits, Stellar Evolution

Scientific paper

The slow envelope detachment of the type that occurs in planetary nebulae is studied under the assumption that the detachment results from increasing radiation pressure. Calculations are carried out for the cases where the mass of the primary is 1.0, 1.5, and 2.0 solar masses, and the mass of the secondary is 0.001, 0.01, and 0.1 solar masses. Applications of the results to V471 Tau, UU Zge, WZ Zge, and the sun-Jupiter system are discussed.

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