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Gravitational detection of a low-mass dark satellite galaxy at cosmological distance

Author
VEGETTI, S1 ; LAGATTUTA, D. J2 ; MCKEAN, J. P3 ; AUGER, M. W4 ; FASSNACHT, C. D2 ; KOOPMANS, L. V. E5
[1] Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, United States
[2] Department of Physics, University of California, Davis, California 95616, United States
[3] ASTRON, Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, Netherlands
[4] Department of Physics, University of California, Santa Barbara, California 93106, United States
[5] Kapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, Netherlands
Source

Nature (London). 2012, Vol 481, Num 7381, pp 341-343, 3 p ; ref : 28 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)
Fonction masse Galaxies compagnons Galaxies naines Galaxies premier type Groupe galaxies Groupe local Matière sombre froide Sous structure
Keyword (en)
Mass function Satellite galaxies Dwarf galaxies Early type galaxies Galaxy groups Local group Cold dark matter Substructure
Keyword (es)
Función masa Galaxias satélite Galaxias primer tipo Materia oscura fría Subestructura
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D65 Galaxy groups, clusters, and superclusters. Large-scale structure of the universe / 001E03D65A Interacting galaxies; galaxy pairs and triples

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
25380621

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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