activity
19992026
most citedPresupernova evolution and explosive nucleosynthesis of rotating massive stars in the metallicity range -3 <=[Fe/H]<= 0

596 citations · 6.1k across the 81 of their papers we have counts for

collaborators
Showing 2003Show all

7 papers · 1 filter

astro-ph2003★ 40 cited

Evolution and nucleosynthesis of primordial low mass stars

I. Picardi, A. Chieffi, M. Limongi +5

We discuss in detail the evolutionary properties of low mass stars M< 1 M(Solar) having metallicity lower than Z=10^(-6) from the pre- main sequence up to (almost) the end of the A…

astro-ph2003

Expected Changes of Supernovae with Redshift due to Evolution of their Progenitors

Inma Dominguez, Peter Hoeflich, Oscar Straniero +2

We have analyzed the influence of the stellar populations, from which SN progenitors come from, on the observational outcome, including the metal free Pop. III. We use our models t…

astro-ph2003★ 50 cited

The Chemical Evolution of Magnesium Isotopic Abundances in the Solar Neighbourhood

Y. Fenner, B. K. Gibson, H. -c. Lee +5

The abundance of the neutron-rich magnesium isotopes observed in metal-poor stars is explained quantitatively with a chemical evolution model of the local Galaxy that considers - f…

astro-ph2003★ 48 cited

Theoretical Light Curves of Type II-P SNe and Applications to Cosmology

A. Chieffi, I. Dominguez, P. Hoeflich +2

Based on an extensive grid of stellar models between 13 and 25 Mo and a wide range of metallicities, we have studied the light curves of core collapse supernovae, their application…

astro-ph2003★ 24 cited

How did the metals in a giant star originate?

Piercarlo Bonifacio, Marco Limongi, Alessandro Chieffi

The chemical composition of stars with extremely low metal contents (taking ``metals'' to mean all elements other than hydrogen and helium) provides us with information on the mass…

astro-ph2003★ 280 cited

Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae

M. Limongi, A. Chieffi

We present a new set of presupernova evolutions and explosive yields of massive stars of initial solar composition (Y=0.285, Z=0.02) in the mass range 13-35 Msun. All the models ha…