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20032009
most citedStellar Models and Yields of Asymptotic Giant Branch Stars

313 citations · 777 across the 12 of their papers we have counts for

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15 papers · 1 filter

astro-ph2008

The impact of the 18F(a,p)21Ne reaction on fluorine production in AGB stars

Amanda I. Karakas, Hye Young Lee, Maria Lugaro +2

The recent experimental evaluation of the 18F(a,p)21Ne reaction rate, when considering its associated uncertainties, presented significant differences compared to the theoretical H…

astro-ph200883 cited

Heavy element abundances in giant stars of the globular clusters M4 and M5

David Yong, Amanda I. Karakas, David L. Lambert +2

We present a comprehensive abundance analysis of 27 heavy elements in bright giant stars of the globular clusters M4 and M5 based on high resolution, high signal-to-noise ratio spe…

astro-ph200859 cited

Chemical abundances in giants stars of the tidally disrupted globular cluster NGC 6712 from high-resolution infrared spectroscopy

David Yong, Jorge Melendez, Katia Cunha +3

We present abundances of C, N, O, F, Na, and Fe in six giant stars of the tidally disrupted globular cluster NGC 6712. The abundances were derived by comparing synthetic spectra wi…

astro-ph200733 cited

The impact of the 18F(a,p)21Ne reaction on asymptotic giant branch nucleosynthesis

Amanda Karakas, Hye Young Lee, Maria Lugaro +2

We present detailed models of low and intermediate-mass asymptotic giant branch (AGB) stars with and without the 18F(a,p)21Ne reaction included in the nuclear network, where the ra…

astro-ph2007

Yields from single AGB stars

Amanda I. Karakas

In order to understand the composition of planetary nebulae we first need to study the nucleosynthesis occurring in the progenitor star during the thermally-pulsing Asymptotic Gian…

astro-ph2007313 cited

Stellar Models and Yields of Asymptotic Giant Branch Stars

Amanda I. Karakas, John C. Lattanzio

We present stellar yields calculated from detailed models of low and intermediate-mass asymptotic giant branch (AGB) stars. We evolve models with a range of mass from 1 to 6Msun, a…