Massive Stars in the Range 13–25 M ⊙ : Evolution and Nucleosynthesis. II. The Solar Metallicity Models | Zendy

Marco Limongi | Zendy; O. Straniero | Zendy; A. Chieffi | Zendy

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Massive Stars in the Range 13–25 M _⊙ : Evolution and Nucleosynthesis. II. The Solar Metallicity Models

Author(s) -

Marco Limongi,

O. Straniero,

A. Chieffi

Publication year - 2000

Publication title -

the astrophysical journal supplement series

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 3.546

H-Index - 277

eISSN - 1538-4365

pISSN - 0067-0049

DOI - 10.1086/313424

Subject(s) - metallicity , nucleosynthesis , astrophysics , physics , stellar evolution , stars , range (aeronautics) , isotope , stellar nucleosynthesis , nuclear physics , materials science , composite material

We present the evolutionary properties of a set of massive stellar models(namely 13, 15, 20 and 25 $\rm M_\odot$) from the main sequence phase up to theonset of the iron core collapse. All these models have initial solar chemicalcomposition, i.e. Y=0.285 and Z=0.02. A 179 isotope network, extending fromneutron up to $\rm ^{68}Zn$ and fully coupled to the evolutionary code has beenadopted from the Carbon burning onward. Our results are compared, wheneverpossible, to similar computations available in literature.Comment: 42 pages, 18 figures, 26 tables, accepted for publicatin in ApJ

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