THE DOUBLE SUBGIANT BRANCH OF NGC 1851 : THE ROLE OF THE CNO ABUNDANCE
- Author
- CASSISI, S1 ; SALARIS, M2 3 ; PIETRINFERNI, A1 ; PIOTTO, G4 ; MILONE, A. P4 ; BEDIN, L. R5 ; ANDERSON, J6
[1] INAF-Osservatorio Astronomico di Collurania, Via M. Maggini, 64100 Teramo, Italy
[2] Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD, United Kingdom
[3] Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, Garching 85748, Germany
[4] Dipartimento di Astronomia, Universitá di Padova, Vicolo dell'Osservatorio 3, 35122 Padua, Italy
[5] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States
[6] Department of Physics and Astronomy, Mail Stop 108, Rice University, 6100 Main Street, Houston, TX 77005, United States - Source
The Astrophysical journal. 2008, Vol 672, Num 2 ; L115-L118 ; 2 ; ref : 1/4 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- English
- Author keyword
- globular clusters: individual (NGC 1851)-Hertzsprung-Russell diagram- stars: abundances stars: evolution
- Keyword (fr)
- Abondance stellaire Amas globulaire Amas stellaire Evolution stellaire Sous géante
- Keyword (en)
- Stellar abundance Globular clusters Star clusters Stellar evolution Subgiant star
- Keyword (es)
- Abundancia estelar Subgigante
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20001273
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
10.1086/527035 
https://dx.doi.org/10.1086/527035
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