Abstract
The presupernova evolutions and the explosive yields of massive stars in the range 13–80 M⊙x withmetallicity Z=0 and Z = 10-3 are presented. Differences in the final elemental yields between the two sets of models are addressed and discussed in terms of differences in the presupernova evolutionary properties. Implications on the enrichment of the interstellar medium for the various generations of stars are also discussed.
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© 2002 Springer Science+Business Media Dordrecht
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Limongi, M., Chieffi, A., Straniero, O., Domínguez, I. (2002). Explosive Yields of Metal-Free SNII and the Abundances in Extremely Metal-Poor Stars. In: Chávez, M., Bressan, A., Buzzoni, A., Mayya, D. (eds) New Quests in Stellar Astrophysics: The Link Between Stars and Cosmology. Astrophysics and Space Science Library, vol 274. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0393-3_40
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DOI: https://doi.org/10.1007/978-94-010-0393-3_40
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3916-1
Online ISBN: 978-94-010-0393-3
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