New asymptotic giant branch models for a range of metallicities
A&A, 508 3 (2009) 1343-1358
Published online: 2009-11-19
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ON THE NECESSITY OF COMPOSITION-DEPENDENT LOW-TEMPERATURE OPACITY IN MODELS OF METAL-POOR ASYMPTOTIC GIANT BRANCH STARS
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HYDRODYNAMIC SIMULATIONS OF H ENTRAINMENT AT THE TOP OF He-SHELL FLASH CONVECTION
Paul R. Woodward, Falk Herwig and Pei-Hung LinThe Astrophysical Journal 798 (1) 49 (2014)
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EVOLUTION OF THERMALLY PULSING ASYMPTOTIC GIANT BRANCH STARS. IV. CONSTRAINING MASS LOSS AND LIFETIMES OF LOW MASS, LOW METALLICITY AGB STARS
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P. Ventura, M. Di Criscienzo, R. Carini and F. D’AntonaMonthly Notices of the Royal Astronomical Society 431 (4) 3642 (2013)
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Planets, Stars and Stellar Systems
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The planetary nebula population in the halo of M 87
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QUIESCENT NUCLEAR BURNING IN LOW-METALLICITY WHITE DWARFS
Marcelo M. Miller Bertolami, Leandro G. Althaus and Enrique García-BerroThe Astrophysical Journal 775 (1) L22 (2013)
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Nucleosynthesis in Stars and the Chemical Enrichment of Galaxies
Ken'ichi Nomoto, Chiaki Kobayashi and Nozomu TominagaAnnual Review of Astronomy and Astrophysics 51 (1) 457 (2013)
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