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19992026
most citedUpdated stellar yields from Asymptotic Giant Branch models

720 citations · 8.5k across the 138 of their papers we have counts for

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Showing 2013Show all

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astro-ph.SR2013★ 59 cited

The impact of updated Zr neutron-capture cross sections and new asymptotic giant branch models on our understanding of the s process and the origin of stardust

Maria Lugaro, Giuseppe Tagliente, Amanda I. Karakas +4

We present model predictions for the Zr isotopic ratios produced by slow neutron captures in C-rich asymptotic giant branch (AGB) stars of masses 1.25 to 4 Msun and metallicities Z…

astro-ph.CO2013★ 278 cited

On the Source of the Dust Extinction in Type Ia Supernovae and the Discovery of Anomalously Strong Na I Absorption

M. M. Phillips, Joshua D. Simon, Nidia Morrell +28

High-dispersion observations of the Na I D 5890, 5896 and K I 7665, 7699 interstellar lines, and the diffuse interstellar band at 5780 Angstroms in the spectra of 32 Type Ia supern…

astro-ph.SR2013

AGB nucleosynthesis at low metallicity: what can we learn from carbon- and s-elements-enhanced metal-poor stars

Carlo Abate, Onno R. Pols, Robert G. Izzard +1

CEMP-s stars are very metal-poor stars with enhanced abundances of carbon and s-process elements. They form a significant proportion of the very metal-poor stars in the Galactic ha…

astro-ph.SR2013★ 9 cited

The Aquarius Co-Moving Group is Not a Disrupted Classical Globular Cluster

Andrew R. Casey, Stefan Keller, Alan Alves-Brito +8

We present a detailed analysis of high-resolution, high S/N spectra for 5 Aquarius stream stars observed with the MIKE spectrograph on the Magellan Clay telescope. Our sample repre…

astro-ph.GA2013★ 76 cited

Metal-Poor Stars Observed with the Magellan Telescope I. Constraints on Progenitor Mass and Metallicity of AGB Stars Undergoing s-Process Nucleosynthesis

Vinicius M. Placco, Anna Frebel, Timothy C. Beers +5

We present a comprehensive abundance analysis of two newly-discovered carbon-enhanced metal-poor (CEMP) stars. HE2138-3336 is a s-process-rich star with [Fe/H] = -2.79, and has the…

astro-ph.SR2013★ 32 cited

Is the Sulphur Anomaly in Planetary Nebulae Caused by the s-Process?

Luke J. Shingles, Amanda I. Karakas

Motivated by unexplained observations of low sulphur abundances in planetary nebulae (PNe) and the PG1159 class of post asymptotic giant branch (AGB) stars, we investigate the poss…