Final phases of stellar evolution and the supernova phenomenon

Details Final phases of stellar evolution and the supernova phenomenon Final phases of stellar evolution and the supernova phenomenon

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48..589g&link_type=abstract

Società Astronomica Italiana, Memorie, vol. 48, Dec. 1977, p. 589-616. In Italian.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Stellar Evolution, Supernovae, Collisions, Degenerate Matter, Eclipsing Binary Stars, Gravitational Collapse, Neutrinos, Nuclear Fusion, Stellar Mass, Stellar Rotation, Stellar Structure, Supermassive Stars, White Dwarf Stars

Scientific paper

Various theoretical aspects of the final stages of stellar evolution are reviewed in the framework of gravitational collapse and thermonuclear reactions (C-12 and O-16) in degenerate electron conditions. Attention is given to the evolution of supermassive stars, massive stars, and low-mass stars and to such topics as neutrino emission in intermediate-mass stars, white-dwarf supernovae, rotational instability, and stellar collisions and eclipsing binary systems.

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