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Carbon deflagration supernova, an alternative to carbon detonation

Abstract

As an alternative to the carbon detonation, a carbon deflagration supernova model is presented 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.
Authors:
Nomoto, K; Sugimoto, D; [1]  Neo, S [2] 
  1. Tokyo Univ. (Japan). Coll. of General Education
  2. Kyoto Univ. (Japan). Dept. of Physics
Publication Date:
Feb 01, 1976
Product Type:
Journal Article
Reference Number:
AIX-07-247054; EDB-76-082943
Resource Relation:
Journal Name: Astrophys. Space Sci.; (Netherlands); Journal Volume: 39:2
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; SUPERNOVAE; HYDRODYNAMICS; STAR MODELS; CARBON; SHOCK WAVES; VELOCITY; WAVE PROPAGATION; ELEMENTS; FLUID MECHANICS; MATHEMATICAL MODELS; MECHANICS; NONMETALS; STARS; 640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources
OSTI ID:
7266960
Country of Origin:
Netherlands
Language:
English
Other Identifying Numbers:
Journal ID: CODEN: APSSB
Submitting Site:
INIS
Size:
Pages: L37-L42
Announcement Date:

Citation Formats

Nomoto, K, Sugimoto, D, and Neo, S. Carbon deflagration supernova, an alternative to carbon detonation. Netherlands: N. p., 1976. Web. doi:10.1007/BF00648354.
Nomoto, K, Sugimoto, D, & Neo, S. Carbon deflagration supernova, an alternative to carbon detonation. Netherlands. doi:10.1007/BF00648354.
Nomoto, K, Sugimoto, D, and Neo, S. 1976. "Carbon deflagration supernova, an alternative to carbon detonation." Netherlands. doi:10.1007/BF00648354. https://www.osti.gov/servlets/purl/10.1007/BF00648354.
@misc{etde_7266960,
title = {Carbon deflagration supernova, an alternative to carbon detonation}
author = {Nomoto, K, Sugimoto, D, and Neo, S}
abstractNote = {As an alternative to the carbon detonation, a carbon deflagration supernova model is presented 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.}
doi = {10.1007/BF00648354}
journal = {Astrophys. Space Sci.; (Netherlands)}
volume = {39:2}
journal type = {AC}
place = {Netherlands}
year = {1976}
month = {Feb}
}