Rotational mixing in low-mass stars

2006/02/17 by A. Palacios, C. Charbonnel, S. Talon +1 · 6 citations
Physics and Astronomy · #Artificial intelligence #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Computer science #Low Mass #Metallicity #Mixing (physics) #Physics #Rotation (mathematics) #Stars #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20053065

21 pages, 16 figures, accepted for publication in Astronomy & Astrophysics

arxiv created 2006/02/17 · openalex publication_date 2006/06/09 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31

Abstract

Aims.In this paper we study the effects of rotation in low-mass, low-metallicity RGB stars.

Citations

• VLT observations of turnoff stars in the globular cluster NGC 6397
• Calibration of the CH and CN Variations Among Main-Sequence Stars in M71 and in M13
• The initial helium abundance of the Galactic globular cluster system
• The Abundance Evolution of Oxygen, Sodium, and Magnesium in Extremely Metal Poor Intermediate-Mass Stars: Implications for the Self-Pollution Scenario in Globular Clusters
• Updated Opal Opacities
• On shear-induced turbulence in rotating stars
• A compilation of charged-particle induced thermonuclear reaction rates
• Mg isotopic ratios in giant stars of the globular cluster NGC 6752
• Comparison between Predicted and Empirical [FORMULA][F]ΔV[SUP][RM]bump[/RM][/SUP][INF][RM]HB[/RM][/INF][/F][/FORMULA] in Galactic Globular Clusters
• The Lithium Flash

Cited by

• Chemical evolution with rotating massive star yields – I. The solar neighbourhood and the s-process elements
• Diagnoses to unravel secular hydrodynamical processes in rotating main sequence stars
• DEEP MIXING AND METALLICITY: CARBON DEPLETION IN GLOBULAR CLUSTER GIANTS
• A model for globular cluster extreme anomalies
• ON LITHIUM-RICH RED GIANTS. I. ENGULFMENT OF SUBSTELLAR COMPANIONS
• Lithium abundances and extra mixing processes in evolved stars of M 67