activity
19982013
most citedThe s-Process in Low Metallicity Stars. II. Interpretation of High-Resolution Spectroscopic Observations with AGB models

248 citations · 657 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2013

CEMP-s and CEMP-s/r stars: last update

S. Bisterzo, R. Gallino, O. Straniero +3

We provide an updated discussion of the sample of CEMP-s and CEMP-s/r stars collected from the literature. Observations are compared with the theoretical nucleosynthesis models of…

astro-ph.SR2012★ 131 cited

s-Process in Low Metallicity Stars. III. Individual analysis of CEMP-s and CEMP-s/r with AGB models

S. Bisterzo, R. Gallino, O. Straniero +2

We provide an individual analysis of 94 carbon enhanced metal-poor stars showing an s-process enrichment (CEMP-s) collected from the literature. The s-process enhancement observed…

astro-ph.SR2011★ 248 cited

The s-Process in Low Metallicity Stars. II. Interpretation of High-Resolution Spectroscopic Observations with AGB models

S. Bisterzo, R. Gallino, O. Straniero +2

High-resolution spectroscopic observations of a hundred metal-poor Carbon and s-rich stars (CEMP-s) collected from the literature are compared with the theoretical nucleosynthesis…

astro-ph2006★ 62 cited

Survival of Nature's Rarest Isotope 180Ta under Stellar Conditions

P. Mohr, F. Kaeppeler, R. Gallino

The nucleosynthesis of nature's rarest isotope 180Ta depends sensitively on the temperature of the astrophysical environment because of depopulation of the long-living isomeric sta…

astro-ph2006★ 182 cited

Sensitivity of p-Process Nucleosynthesis to Nuclear Reaction Rates in a 25 Solar Mass Supernova Model

W. Rapp, J. Goerres, M. Wiescher +2

The astrophysical p process, which is responsible for the origin of the proton rich stable nuclei heavier than iron, was investigated using a full nuclear reaction network for a ty…

astro-ph2004★ 32 cited

128Xe and 130Xe: Testing He-shell burning in AGB stars

R. Reifarth, F. Kaeppeler, F. Voss +4

The s-process branching at 128I has been investigated on the basis of new, precise experimental (n,g) cross sections for the s-only isotopes 128Xe and 130Xe. This branching is uniq…