Beryllium in turnoff stars of NGC 6397: Early Galaxy spallation, cosmochronology and cluster formation
- 11 October 2004
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 426 (2) , 651-657
- https://doi.org/10.1051/0004-6361:20041254
Abstract
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysicsKeywords
All Related Versions
This publication has 28 references indexed in Scilit:
- Nitrogen abundances in planet-harbouring starsAstronomy & Astrophysics, 2004
- First stars V - Abundance patterns from C to Zn and supernova yields in the early GalaxyAstronomy & Astrophysics, 2004
- First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic ResultsThe Astrophysical Journal Supplement Series, 2003
- The lithium content of the globular cluster NGC 6397Astronomy & Astrophysics, 2002
- Evolution and Nucleosynthesis of Zero‐Metal Intermediate‐Mass StarsThe Astrophysical Journal, 2001
- Beryllium Abundances in Halo Stars from Keck/HIRES ObservationsThe Astronomical Journal, 1999
- Is beryllium in metal-poor stars of galactic or cosmological origin?Nature, 1992
- Carbon and nitrogen abundances in metal-poor dwarfs of the solar neighborhoodPublications of the Astronomical Society of the Pacific, 1987
- Nitrogen overabundances in Population II dwarfsThe Astrophysical Journal, 1982
- Lithium and the s-PROCESS in Red-Giant StarsThe Astrophysical Journal, 1971