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Chemical abundances of late-type pre-main sequence stars in the σOrionis cluster
- Source :
- Astronomy and Astrophysics; November 2008, Vol. 490 Issue: 3 p1135-1142, 8p
- Publication Year :
- 2008
-
Abstract
- Context. The young σOrionis cluster is an important location for studying the formation and evolution of stars, brown dwarfs, and planetary-mass objects. Its metallicity, although it is a fundamental parameter, has not been well determined yet.
Details
- Language :
- English
- ISSN :
- 00046361 and 14320746
- Volume :
- 490
- Issue :
- 3
- Database :
- Supplemental Index
- Journal :
- Astronomy and Astrophysics
- Publication Type :
- Periodical
- Accession number :
- ejs53157400
- Full Text :
- https://doi.org/10.1051/0004-6361:200810398