Presupernova evolution of massive stars

Physics Reports

Volumn 163, Issue 1-3, 1988, Pages 13-36

  Nomoto, Ken'ichi ^a,b   Hashimoto, Masa aki ^a,b,c  

^a UNIVERSITY OF TOKYO   (Japan)

^b BROOKHAVEN NATIONAL LABORATORY   (United States)

^c MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001971387     PISSN: 03701573     EISSN: None     Source Type: Journal    
DOI: 10.1016/0370-1573(88)90032-4     Document Type: Article

References (48)

1. Stars in the mass ratio range from 7 to 10 as candidates for pulsar progenitors
2. Collapse of 9 solar mass stars
3. The prompt mechanism of Type II supernovae
4. A comparative study of supernova light curves
5. Stellar weak-interaction rates for sd-shell nuclei. I - Nuclear matrix element systematics with application to Al-26 and selected nuclei of importance to the supernova problem
6. Stellar weak interaction rates for intermediate mass nuclei. III - Rate tables for the free nucleons and nuclei with A = 21 to A = 60
7. Thermonuclear Reaction Rates, III
8. Accreting white dwarf models for type I supernovae. I - Presupernova evolution and triggering mechanisms
9. Evolution of 8-10 solar mass stars toward electron capture supernovae. I - Formation of electron-degenerate O + NE + MG cores
10. Evolution of Supernova Progenitors and Supernova Models
11. Evolution of 8-10 solar mass stars toward electron capture supernovae. II - Collapse of an O + NE + MG core
12. Proc. Japan-France Seminar on Chemical Evolution of Galaxies with Active Star Formation
13. White dwarf models of supernovae and cataclysmic variables
14. Accreting white dwarf models of Type I supernovae. III - Carbon deflagration supernovae
15. Hydrostatic Nucleosynthesis - Part Two - Core Neon to Silicon Burning and Presupernova Abundance Yields of Massive Stars
16. Ultraviolet spectral evolution and heavy element abundances in Nova Austrinae 1981
17. The Physics of Supernova Explosions