A double stellar generation in the globular cluster NGC 6656 (M 22): Two stellar groups with different iron and s-process element abundances
- Author
- MARINO, A. F1 2 ; MILONE, A. P1 ; PIOTTO, G1 ; VILLANOVA, S3 ; BEDIN, L. R4 ; BELLINI, A1 4 ; RENZINI, A5
[1] Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 3, 35122 Padova, Italy
[2] P. Universidad Católica de Chile, Departamento de Astronomia y Astrofisica, Casilla 306, Santiago, Chile
[3] Departamento de Astronomia, Universidad de Concepcion, Casilla 160-C, Concepcion, Chile
[4] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States
[5] Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy - Source
Astronomy and astrophysics (Berlin. Print). 2009, Vol 505, Num 3, pp 1099-1113, 15 p ; ref : 1/2 p
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- galaxy: globular clusters: individual: NGC 6656 stars: abundances
- Keyword (fr)
- Abondance stellaire Abondance élément Amas galaxies Amas globulaire Amas stellaire Anticorrélation Etoile M Etoile S Etoile brillante Etoile géante Population stellaire Processus r Processus s
- Keyword (en)
- Stellar abundance Element abundance Galaxy clusters Globular clusters Star clusters Anticorrelation M stars S stars Bright star Giant stars Stellar population r process s process
- Keyword (es)
- Abundancia estelar Anticorrelación Estrella brillante Población estelar
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 22053257
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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