Microscopic calculation of the rates of electron captures which induce the collapse of O+Ne+Mg cores
- 1 November 1989
- journal article
- Published by Elsevier in Nuclear Physics A
- Vol. 504 (1) , 167-192
- https://doi.org/10.1016/0375-9474(89)90288-1
Abstract
No abstract availableThis publication has 17 references indexed in Scilit:
- Presupernova evolution of massive starsPhysics Reports, 1988
- Evolution of 8-10 solar mass stars toward electron capture supernovae. II - Collapse of an O + NE + MG coreThe Astrophysical Journal, 1987
- On the collapse of 8-10 solar mass stars due to electron captureThe Astrophysical Journal, 1987
- Experimental and theoretical Gamow-Teller beta-decay observables for the sd-shell nucleiAtomic Data and Nuclear Data Tables, 1985
- Gamow-Teller electron capture strength distributions in stars: Unblocked iron and nickel isotopesNuclear Physics A, 1985
- Evolution of 8-10 solar mass stars toward electron capture supernovae. I - Formation of electron-degenerate O + NE + MG coresThe Astrophysical Journal, 1984
- Stellar weak interaction rates for intermediate-mass nuclei. II - A = 21 to A = 60The Astrophysical Journal, 1982
- Equation of state in the gravitational collapse of starsNuclear Physics A, 1979
- Decay of24Al and24Almto γ-Ray and α-Particle Emitting States in24MgPhysica Scripta, 1979
- Beta-decay half-lives calculated on the gross theoryAtomic Data and Nuclear Data Tables, 1973