On the formation and evolution of magnetic chemically peculiar stars in the solar neighborhood
- Author
- PÖHNL, H1 ; PAUNZEN, E1 ; MAITZEN, H. M1
[1] Institut für Astronomie der Universität Wien, Türkenschanzstr. 17, 1180 Wien, Austria - Source
Astronomy and astrophysics (Berlin. Print). 2005, Vol 441, Num 3, pp 1111-1116, 6 p ; ref : 41 ref
- 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
- stars: chemically peculiar stars: evolution stars: fundamental parameters
- Keyword (fr)
- Age Champ intense Champ magnétique Champ température Classification Couleur Durée vie Etoile K Etoile chimiquement particulière Etoile magnétique Etoile séquence principale Evolution stellaire Formation stellaire Modèle Perte moment cinétique Soleil Sous groupe Température critique Température effective Voisinage solaire
- Keyword (en)
- Age High field Magnetic fields Temperature distribution Classification Color Lifetime K stars Chemically peculiar star Magnetic stars Main sequence stars Stellar evolution Star formation Models Angular momentum loss Sun Subgroup Critical temperature Effective temperature Solar neighborhood
- Keyword (es)
- Edad Estrella quimicamente particular Modelo Perdidad momento angular Subgrupo Vecindad solar
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 17142284
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
10.1051/0004-6361:20053272 
https://dx.doi.org/10.1051/0004-6361:20053272
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