A spectroscopic survey of WNL stars in the Large Magellanic Cloud : general properties and binary status
- Author
- SCHNURR, O1 2 3 ; MOFFAT, A. F. J1 2 ; ST-LOUIS, N1 2 ; MORRELL, N. I4 ; GUERRERO, M. A5
[1] Dépt. de Physique, Université de Montréal, C. P. 6128, succ. centre-ville, Montréal (Qc) H3C 3J7, Canada
[2] Centre de Recherche en Astrophysique du Québec, Canada
[3] Department of Physics and Astronomy, University of Sheffield, Hicks Building Hounsfield Road, Sheffield S3 7RH, United Kingdom
[4] Las Campanas Observatory, Observatories of the Carnegie Institution of Washington, Casilla 601, La Serena, Chile
[5] Instituto de Astrofisica de Andalucia, Consejo Superior de Investigaciones Cientificas, Apartado Correos 3004, 18080 Granada, Spain - Source
Monthly Notices of the Royal Astronomical Society. 2008, Vol 389, Num 2, pp 806-828, 23 p ; ref : 3/4 p
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Blackwell Science, Oxford
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- Magellanic Clouds binaries: general stars: Wolf-Rayet stars: evolution
- Keyword (fr)
- Combustion hydrogène Combustion hélium Combustion stellaire Etoile hélium Etoile massive Etoile type Wolf Rayet Evolution stellaire Grand Nuage Magellan Groupe local Luminosité Modèle Nuages Magellan Observable Orbite Photométrie Variabilité Vitesse radiale Voie lactée
- Keyword (en)
- Hydrogen burning Helium burning Star burning Helium stars Massive stars Wolf-Rayet stars Stellar evolution Large Magellanic Cloud Local group Luminosity Models Magellanic Clouds Observables Orbits Photometry Variability Radial velocity Milky Way
- Keyword (es)
- Modelo Variabilidad
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20618447
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
10.1111/j.1365-2966.2008.13584.x 
https://dx.doi.org/10.1111/j.1365-2966.2008.13584.x
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