New light on the formation and evolution of M 31 and its globular cluster system
- Author
- PUZIA, T. H1 ; PERRETT, K. M2 ; BRIDGES, T. J3
[1] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States
[2] Department of Astronomy & Astrophysics, University of Toronto, Toronto, ON, M5S 3H8, Canada
[3] Department of Physics, Queen's University, Kingston, ON, K7L 3N6, Canada - Source
Astronomy and astrophysics (Berlin. Print). 2005, Vol 434, Num 3, pp 909-934, 26 p ; ref : 1 p.3/4
- 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: general galaxies: Local Group galaxies: evolution galaxies: formation galaxies: general galaxies: star clusters
- Keyword (fr)
- Abondance solaire Age Amas galactique Amas galaxies Amas globulaire Amas stellaire Cinématique Corrélation croisée Formation galaxies Galaxies spirales Grand Nuage Magellan Groupe galaxies Groupe local Interpolation Modèle Métallicité Population stellaire Raie Balmer Rapport abondance Voie lactée Evolution galaxies
- Keyword (en)
- Solar abundance Age Galactic cluster Galaxy clusters Globular clusters Star clusters Kinematics Cross correlations Galaxy formation Spiral galaxies Large Magellanic Cloud Galaxy groups Local group Interpolation Models Metallicity Stellar population Balmer lines Abundance ratio Milky Way Galaxy evolution
- Keyword (es)
- Abundancia solar Edad Conglomerado galáctico Modelo Metalicidad Población estelar Relación abundancia Evolución galaxias
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 16711783
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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DOI
10.1051/0004-6361:20041813 
https://dx.doi.org/10.1051/0004-6361:20041813
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