Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..39l..37n&link_type=abstract
Astrophysics and Space Science, vol. 39, Feb. 1976, p. L37-L42. Research supported by the Ministry of Education and Japan Societ
Astronomy and Astrophysics
Astrophysics
131
Carbon, Nuclear Fusion, Stellar Evolution, Supernovae, Wave Propagation, Convective Heat Transfer, Stellar Models, Thermal Instability
Scientific paper
As an alternative to the carbon detonation, the paper presents a carbon deflagration supernova model by a full hydrodynamic computation. A deflagration wave, which propagates through the core due to convective heat transport, does not grow into detonation. Though it results in a complete disruption of the star, the difficulty of overproduction of iron peak elements can be avoided if the deflagration is relatively slow.
Neo S.
Nomoto Ken
Sugimoto Daiichiro
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