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A substantial population of low-mass stars in luminous elliptical galaxies

Author
VAN DOKKUM, Pieter G1 ; COMOY, Charlie2 3
[1] Astronomy Department, Yale University, New Haven, Connectitcut, United States
[2] Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey, United States
[3] Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts, United States
Source

Nature (London). 2010, Vol 468, Num 7326, pp 940-942, 3 p ; ref : 30 ref

CODEN
NATUAS
ISSN
0028-0836
Scientific domain
Multidisciplinary
Publisher
Nature Publishing Group, London
Publication country
United Kingdom
Document type
Article
Language
English
Keyword (fr)
Cosmologie Disque galactique Distribution masse Etoile faible masse Etoile massive Fonction masse initiale Galaxies elliptiques Rapport signal bruit Spectre IR Univers primordial
Keyword (en)
Cosmology Galactic disks Mass distribution Low-mass stars Massive stars Initial mass function Elliptical galaxies Signal-to-noise ratio Infrared spectra Early universe
Keyword (es)
Función masa inicial
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D52 Normal galaxies. Extragalactic objects and systems (by type) / 001E03D52E Elliptical galaxies

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D62 Characteristics and properties of external galaxies and extragalactic objects / 001E03D62L Stellar content and populations. Radii. Morphology and overall structure

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
23529502

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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