The evolution of massive stars
Hydrogen exhaustion through the onset of carbon burning / by Chushiro Hayashi and Robert C. Cameron
1962
III, 40 S.
3
Miscellaneous
English
RVK: | ZO 7000 |
Neutrino cooling rates due to 54,55,56Fe for presupernova evolution of massive stars
Online Contents | 2011
|Light Element Production by Low Energy Nuclei from Massive Stars
British Library Online Contents | 1997
|Ganma-Ray Lines and LiBeB from Massive Stars: II. WC Explosion
British Library Online Contents | 1997
|Gamma-Ray Lines and LiBeB from Massive Stars: III. SNR Expansion
British Library Online Contents | 1997
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