On a physical mechanism for extra mixing in globular cluster red giants
Open Access
- 1 August 2000
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 316 (2) , 395-406
- https://doi.org/10.1046/j.1365-8711.2000.03498.x
Abstract
No abstract availableKeywords
This publication has 23 references indexed in Scilit:
- Proton Capture Chains in Globular Cluster Stars.II.Oxygen, Sodium, Magnesium, and Aluminum Abundances in M13 Giants Brighter Than the Horizontal BranchThe Astronomical Journal, 1997
- A Consistent Explanation for [TSUP]12[/TSUP]C/[TSUP]13[/TSUP]C, [TSUP]7[/TSUP]Li, and [TSUP]3[/TSUP]He Anomalies in Red Giant StarsThe Astrophysical Journal, 1995
- On the Interaction of Convection and Rotation in StarsThe Astrophysical Journal, 1995
- Rotation and Oxygen Line Strengths in Blue Horizontal-Branch StarsThe Astrophysical Journal, 1995
- Far-ultraviolet photometry of the globular cluster omega CENThe Astronomical Journal, 1994
- Sodium-oxygen abundance anticorrelations and deep-mixing scenarios for globular-cluster giantsPublications of the Astronomical Society of the Pacific, 1993
- Thermonuclear reaction rates VAtomic Data and Nuclear Data Tables, 1988
- On the carbon abundance of subgiant stars in the globular cluster M 92Publications of the Astronomical Society of the Pacific, 1986
- Carbon abundances in red giant stars in the globular clusters M92 and NGC 6397The Astrophysical Journal, 1979
- Zum Strahlungsgleichgewicht der SterneAstronomische Nachrichten, 1924