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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DOI
10.1038/nature09578 
https://dx.doi.org/10.1038/nature09578
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