TY - JOUR
T1 - Presupernova evolution and explosive nucleosynthesis of zero metal massive stars
AU - Limongi, Marco
AU - Chieffi, Alessandro
PY - 2012
Y1 - 2012
N2 - We present a new set of zero metallicity models in the range 13-80 M-circle dot together to the associated explosive nucleosynthesis. These models are fully homogeneous with the solar metallicity set we published in Limongi Chieffi and will be freely available at the Online Repository for the FRANEC Evolutionary Output Web site. A comparison between these yields and an average star that represents the average behavior of most of the very metal-poor stars in the range -5.0 <[Fe/H] <-2.5 confirms previous findings that only a fraction of the elemental [X/Fe] may be fitted by the ejecta of standard core collapse supernovae.
AB - We present a new set of zero metallicity models in the range 13-80 M-circle dot together to the associated explosive nucleosynthesis. These models are fully homogeneous with the solar metallicity set we published in Limongi Chieffi and will be freely available at the Online Repository for the FRANEC Evolutionary Output Web site. A comparison between these yields and an average star that represents the average behavior of most of the very metal-poor stars in the range -5.0 <[Fe/H] <-2.5 confirms previous findings that only a fraction of the elemental [X/Fe] may be fitted by the ejecta of standard core collapse supernovae.
UR - http://adsabs.harvard.edu/abs/2012ApJS..199...38L
UR - https://www.scopus.com/pages/publications/84860157386
U2 - 10.1088/0067-0049/199/2/38
DO - 10.1088/0067-0049/199/2/38
M3 - Article
SN - 0067-0049
VL - 199
SP - 1
EP - 9
JO - The Astrophysical Journal Supplement Series
JF - The Astrophysical Journal Supplement Series
IS - 2
ER -