AmFm and lithium gap stars: Stellar evolution models with mass loss
- Author
- VICK, M1 3 ; MICHAUD, G2 3 ; RICHER, J3 ; RICHARD, O1
[1] GRAAL UMR 5024, Université Montpellier II, CC072, Place E. Bataillon, 34095 Montpellier, France
[2] LUTH, Observatoire de Paris, CNRS, Université Paris Diderot, 5 place Jules Janssen, 92190 Meudon, France
[3] Département de physique, Université de Montréal, Montréal, Québec, H3C 3J7, Canada - Source
Astronomy and astrophysics (Berlin. Print). 2010, Vol 521 ; A62.1-A62.26 ; ref : 1 p.1/4
- 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
- diffusion open clusters and associations: individual: Hyades stars: abundances stars: chemically peculiar stars: evolution stars: mass-loss
- Keyword (fr)
- Abondance stellaire Accélération radiative Amas ouvert Amas stellaire Anomalie Diffusion(transport) Durée vie Etoile F Etoile Fm Etoile M Etoile chimiquement particulière Etoile froide Evolution stellaire Masse stellaire Modèle stellaire Mélangeage Opacité Perte masse Taux perte
- Keyword (en)
- Stellar abundance Radiative acceleration Open clusters Star clusters Anomaly Diffusion Lifetime F stars Fm stars M stars Chemically peculiar star Cool star Stellar evolution Stellar mass Star models Mixing Opacity Mass loss Loss rate
- Keyword (es)
- Abundancia estelar Aceleración radiativa Anomalía Estrella quimicamente particular Estrella fría Porcentaje pérdida
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 23727104
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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