Abundances of C, N, O in slightly evolved stars in the globular clusters NGC 6397, NGC 6752 and 47 Tuc
Open Access
- 22 March 2005
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 433 (2) , 597-611
- https://doi.org/10.1051/0004-6361:20041892
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 45 references indexed in Scilit:
- The Chemical Inhomogeneity of Faint M13 Stars: Carbon and Nitrogen AbundancesThe Astronomical Journal, 2004
- On the Carbon and Nitrogen Abundances of 47 Tucanae's Main-Sequence StarsThe Astronomical Journal, 2004
- Carbon Abundances of Faint Stars in M13: Evidence of Two Abundance-altering MechanismsThe Astrophysical Journal, 2002
- The lithium content of the globular cluster NGC 6397Astronomy & Astrophysics, 2002
- Models for Old, Metal‐poor Stars with Enhanced α‐Element Abundances. III. Isochrones and Isochrone Population FunctionsThe Astrophysical Journal, 2001
- Calibration of the CH and CN Variations Among Main-Sequence Stars in M71 and in M13The Astronomical Journal, 2001
- Carbon Abundances of M92 Red Giant Branch StarsPublications of the Astronomical Society of the Pacific, 2001
- Abundance trends among neutron capture elements in giants of globular clusters M5, M3, M13, M92, and M15The Astronomical Journal, 1994
- An analysis of G-band strengths in NGC 6397 and M55 red giantsThe Astrophysical Journal, 1990
- Abundances of the elements: Meteoritic and solarGeochimica et Cosmochimica Acta, 1989