Dynamical friction on galactic center star clusters with an intermediate-mass black hole
- Autor
- KIM, Sungsoo S1 ; FIGER, Donald F2 ; MORRIS, Mark3
[1] Department of Astronomy and Space Science and Institute of Natural Sciences, Kyung Hee University, Yongin-shi, Kyungki-do 449-701, Korea, Republic of
[2] Space Telescope Science Institute, 37(X) San Martin Drive, Baltimore, MD 21218, United States
[3] Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1562, United States - Fuente
The Astrophysical journal. 2004, Vol 607, Num 2, pp L123-L126 ; 2 ; ref : 21 ref
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Campo Científico
- Astronomy earth cosmic environment
- Editor
- University of Chicago Press, Chicago, IL
- País de la publicación
- United States
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave (fr)
- Amas galactique Amas stellaire Centre galactique Cosmologie Dynamique stellaire Etoile jeune Frottement dynamique Simulation numérique Système n corps Trou noir
- Palabra clave (in)
- Galactic cluster Star clusters Galactic centers Cosmology Stellar dynamics Young stars Dynamical friction Digital simulation N body system Black holes
- Palabra clave (es)
- Conglomerado galáctico Frotamiento dinámico Sistema n cuerpos
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D35 Characteristics and properties of the milky way / 001E03D35J Galactic center, bar, circumnuclear matter, and bulge (including black hole and distance measurements)
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D35 Characteristics and properties of the milky way / 001E03D35L Stellar content and populations. Morphology and overall structure
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 15959240
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
10.1086/422032 
https://dx.doi.org/10.1086/422032
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