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Is there a chance for primordial SNeI1/2?
Proceedings of Supernovae: lights in the darkness — PoS(SUPERNOVA)
The evolution of primordial stars of initial masses between 5 and 10 M ⊙ has been computed and analyzed in order to determine the nature of the remnants of massive intermediate-mass primordial stars and to check the influence of overshooting in their evolution. We have obtained the values for the limiting masses of Population III progenitor stars leading to carbon-oxygen and oxygen-neon compact cores. We have also obtained the limiting mass for which isolated primordial stars would lead todoi:10.22323/1.060.0013 fatcat:26d6c54lyjfwzbb7s2tqlbcjta