The magnetohydrodynamic rotational model of supernova explosion
- 1 June 1976
- journal article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 41 (2) , 287-320
- https://doi.org/10.1007/bf00646184
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- On the Possibility of Neutron-Star Formation in Carbon-Detonation SupernovaeThe Astrophysical Journal, 1973
- Nonlinear Landau Damping of Alfvén WavesPhysical Review Letters, 1971
- Density fluctuations driven by Alfvén wavesJournal of Geophysical Research, 1971
- Thermonuclear Detonations in Evolved Stellar CoresThe Astrophysical Journal, 1971
- Do Pulsars Make Supernovae?The Astrophysical Journal, 1971
- A Numerical Example of the Collapse of a Rotating Magnetized StarThe Astrophysical Journal, 1970
- A possible model of supernovae: Detonation of12CAstrophysics and Space Science, 1969
- MASS DEPENDENCE IN GRAVITATIONAL COLLAPSE OF STELLAR CORESCanadian Journal of Physics, 1967
- The Hydrodynamic Behavior of Supernovae ExplosionsThe Astrophysical Journal, 1966
- Neutrino Processes and Pair Formation in Massive Stars and Supernovae.The Astrophysical Journal Supplement Series, 1964