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On the origin of the radial mass density profile of the Galactic halo globular cluster system

Author
PARMENTIER, Geneviève1 ; GREBEL, Eva K1
[1] Astronomical Institute, University of Basel, 7 Venusstrasse, 4102 Binningen, Switzerland
Source

Monthly Notices of the Royal Astronomical Society. 2005, Vol 359, Num 2, pp 615-623, 9 p ; ref : 47 ref

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
Galaxy: formation Galaxy: halo globular clusters: general
Keyword (fr)
Age Amas galactique Amas globulaire Aplatissement Centre galactique Distribution masse Evaporation Fonction masse initiale Gaz chaud Gaz froid Halo galactique Matière sombre Proto galaxie Répartition spatiale Voie lactée
Keyword (en)
Age Galactic cluster Globular clusters Flattening Galactic centers Mass distribution Evaporation Initial mass function Hot gas Cold gas Galactic halos Dark matter Proto galaxy Spatial distribution Milky Way
Keyword (es)
Edad Conglomerado galáctico Aplanamiento Función masa inicial Gas caliente Gas frío Proto galaxia
Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16742516

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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