Late-type red supergiants : Too cool for the magellanic clouds?
- Author
- LEVESQUE, Emily M1 ; MASSEY, Philip2 ; OLSEN, K. A. G3 ; PLEZ, Bertrand4
[1] Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, United States
[2] Lowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ 86001, United States
[3] Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile
[4] GRAAL, Université Montpellier II, CNRS, 34095 Montpellier, France - Source
The Astrophysical journal. 2007, Vol 667, Num 1, pp 202-212, 11 p ; 1 ; ref : 1/2 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
- stars: late-type stars: mass loss stars: évolution supergiants
- Keyword (fr)
- Etoile type avancé Evolution stellaire Masse stellaire Nuages Magellan Perte masse Supergéante rouge
- Keyword (en)
- Late type stars Stellar evolution Stellar mass Magellanic Clouds Mass loss Red supergiant
- Keyword (es)
- Supergigante roja
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 19095301
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
10.1086/520797 
https://dx.doi.org/10.1086/520797
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