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pro vyhledávání: '"F. J. Barrón de Angoiti"'
Autor:
F. J. Barrón de Angoiti
Publikováno v:
Astrophysics and Space Science. 169:149-151
Star evolution at constant mass is typically considered as well defined, given initial mass and composition. However, in the stellar mass range of 8–10M⊙, large uncertainties — as to the treatment of convection and hydrodynamical burning, or th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::672c573e29b128cdfb82cec5bd18e626
https://doi.org/10.1007/bf00640702
https://doi.org/10.1007/bf00640702
