The composite-spectrum binary hypothesis does not explain the λ Bootis stars
- Author
- GRIFFIN, R. E1 ; GRAY, R. O2 ; CORBALLY, C. J3
[1] Dominion Astrophysical Observatory, 5071 West Saanich Road, Victoria, BC, V9E 2E7, Canada
[2] Department of Physics and Astronomy, Appalachian State University, Boone, NC 28608, United States
[3] Vatican Observatory Research Group, Steward Observatory, Tucson, AZ 85721-0065, United States - Source
Astronomy and astrophysics (Berlin. Print). 2012, Vol 547 ; A8.1-A8.14 ; 1 ; ref : 1/4 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
- binaries: spectroscopic stars: chemically peculiar stars: early-type stars: individual: λ Bootis
- Keyword (fr)
- Abondance solaire Binaire spectroscopique Classification Etoile Ap Etoile Be Etoile chimiquement particulière Etoile premier type Etoile type lambda Bootis Modèle Profil raie Propriété physique Spectrométrie Type spectral Variation rapide Vitesse radiale
- Keyword (en)
- Solar abundance Spectroscopic binary stars Classification Ap stars Be stars Chemically peculiar star Early type stars Lambda Bootis stars Models Line shape Physical properties Spectroscopy Spectral type Fast variation Radial velocity
- Keyword (es)
- Abundancia solar Estrella quimicamente particular Modelo Tipo espectral Variación rápida
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 26783887
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
10.1051/0004-6361/201219112 
https://dx.doi.org/10.1051/0004-6361/201219112
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