The common envelope phase in classical novae - One-dimensional models

Details The common envelope phase in classical novae - One-dimensional models The common envelope phase in classical novae - One-dimensional models

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...374..623s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 374, June 20, 1991, p. 623-630. Research supported by Technion - Israel Ins

Astronomy and Astrophysics

Astrophysics

23

Binary Stars, Novae, Stellar Envelopes, Stellar Models, White Dwarf Stars, Missing Mass (Astrophysics), Stellar Radiation, X Rays

Scientific paper

The effects of energy deposition due to the motion of the secondary in an expanding nova envelope are explored for 1 solar mass white dwarfs. Results of one-dimensional hydrodynamic calculations show that a common envelope phase can significantly accelerate mass loss from the system, thereby altering the outburst character. Such a rapid mass loss is necessary in order to explain the early appearance of a nebular spectrum and of X-ray emission, in a number of observed systems.

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