White dwarf evolutionary sequences for low-metallicity progenitors: The impact of third dredge-up

2015/02/13 by L. G. Althaus, Leandro G. Althaus, María E. Camisassa +6 · 107 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics #Biology #Context (archaeology) #Gamma-ray bursts and supernovae #Gene #Genetics #Metallicity #Paleontology #Physics #Progenitor #Progenitor cell #Stars #Stellar, planetary, and galactic studies #Stem cell #White (mutation) #White dwarf #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201424922

published in Astronomy and Astrophysics 576, A9 (EDP Sciences) · To be published in Astronomy and Astrophysics. 12 pages, 11 figures

arxiv created 2015/02/13 · openalex publication_date 2015/02/20 · arxiv updated 2015/06/23 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context. White dwarfs are nowadays routinely used as reliable cosmochronometers, allowing several stellar populations to be dated.

Citations

• Outer boundary conditions for evolving cool white dwarfs
• The Pulsating White Dwarf Stars
• An age difference of two billion years between a metal-rich and a metal-poor globular cluster
• Evolutionary and pulsational properties of white dwarf stars
• Turbulent Convection in Stellar Interiors. I. Hydrodynamic Simulation
• Updated Opal Opacities
• New evolutionary models for massive ZZ Ceti stars. I. First results for their pulsational properties
• A compilation of charged-particle induced thermonuclear reaction rates
• Low‐Temperature Opacities

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