Steady mass loss associated with nova outbursts

Details Steady mass loss associated with nova outbursts Steady mass loss associated with nova outbursts

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..99..295k&link_type=abstract

(International Astronomical Union, Colloquium on Double Stars, Physical Properties and Generic Relations, 80th, Bandung, Indones

Astronomy and Astrophysics

Astrophysics

2

Novae, Stellar Envelopes, Stellar Mass Ejection, White Dwarf Stars, Steady State, Stellar Luminosity, Thermonuclear Reactions

Scientific paper

The structure of optically thick mass-losing envelopes of white dwarfs
are studied in relation to nova outbursts. A sequence of steady
mass-loss solutions is constructed for a nova outburst from the maximum
photospheric radius to the disappearance. Much of mass of the envelope
will be blown out.

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