Computer Science
Scientific paper
Jun 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8028279s&link_type=abstract
"Nature of type 1 Supernovae Transl. into ENGLISH of "O Prirode Sverhnovykh i Tipa'', Rept. Pr-395 Acad. of Sci. USSR, Inst. o
Computer Science
Stellar Evolution, Supernova Remnants, Supernovae, Binary Stars, Elliptical Galaxies, Neutron Stars, Planetary Nebulae, Spiral Galaxies, Stellar Envelopes, Stellar Mass, White Dwarf Stars
Scientific paper
The nature of type 1 supernovae (SN 1) is discussed through a comparison of observational evidence and theoretical perspectives relating to both type 1 and 2 supernovae. In particular two hypotheses relating to SN 1 phenomenon are examined: the first proposing that SN 1 are components of binary systems in which, at a comparatively late stage of evolution, overflow of the mass occurs; the second considers pre-SN 1 to be recently evolved stars with a mass greater than 1.4 solar mass (white dwarfs). In addition, an explanation of the reduced frequency of flares of SN 1 in spiral galaxies as related to that in elliptical galaxies is presented.
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