Rapid formation of supermassive black hole binaries in galaxy mergers with gas
- Author
- MAYER, L; KAZANTZIDIS, S; MADAU, P; COLPI, M; QUINN, T; WADSLEY, J
- Source
Science (Washington, D.C.). 2007, Vol 316, Num 5833, pp 1874-1877, 4 p ; ref : 31 ref
- CODEN
- SCIEAS
- ISSN
- 0036-8075
- Scientific domain
- Multidisciplinary
- Publisher
- American Association for the Advancement of Science, Washington, DC
- Publication country
- United States
- Document type
- Article
- Language
- English
- Keyword (fr)
- Cosmologie Galaxies en coalescence Galaxies en interaction Galaxies spirales Modèle hydrodynamique Modélisation Noyau galaxies Onde gravitationnelle Simulation numérique Trou noir supermassif Trou noir
- Keyword (en)
- Cosmology Merging galaxies Interacting galaxies Spiral galaxies Hydrodynamic model Modelling Galaxy nuclei Gravitational waves Digital simulation Supermassive black hole Black holes
- Keyword (es)
- Galaxias en coalescencia Agujero negro supermasivo
- Classification
- 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 / 001E03D62J Galactic nuclei (including black holes), circumnuclear matter, and bulges
- 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 / 001E03D65F Galaxy mergers, collisions, and tidal interactions
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18929389
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
10.1126/science.1141858 
https://dx.doi.org/10.1126/science.1141858
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