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A semi-empirical study of the mass distribution of horizontal branch stars in M 3 (NGC 5272)

Author
VALCARCE, A. A. R1 ; CATELAN, M1
[1] Pontificia Universidad Católica de Chile, Departamento de Astronomia y Astrofisica, Av. Vicuña Mackena 4860, 782-0436 Macul, Santiago, Chile
Source

Astronomy and astrophysics (Berlin. Print). 2008, Vol 487, Num 1, pp 185-195, 11 p ; 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
Galaxy: globular clusters: individual: M 3 stars: evolution stars: horizontal-branch
Keyword (fr)
Age Amas galaxies Amas globulaire Amas stellaire Composition chimique Couleur Diagramme magnitude couleur Distribution masse Etoile M Etoile S Etoile branche horizontale Evolution stellaire Géante rouge Mode propre Modèle Moment statistique Observation photométrique Perte masse
Keyword (en)
Age Galaxy clusters Globular clusters Star clusters Chemical composition Color Color-magnitude diagrams Mass distribution M stars S stars Horizontal-branch stars Stellar evolution Red giant stars Eigenmode Models Statistical moment Photometric observation Mass loss
Keyword (es)
Edad Modo propio Modelo Momento estadístico Observación fotométrica
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20535731

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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