Evolution of growing black holes in axisymmetric galaxy cores
- Autor
- FIESTAS, J1 2 ; PORTH, O3 ; BERCZIK, P1 2 4 ; SPURZEM, R1 2 5
[1] Zentrum für Astronomie der Universität Heidelberg, Astronomisches Rechen-Institut, Mönchhofstrasse 12-14, 69120 Heidelberg, Germany
[2] National Astronomical Observatories of China, Chinese Academy of Sciences NAOC/CAS, 20A Datun Rd., Chaoyang District, Beijing 100012, China
[3] Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
[4] Main Astronomical Observatory, National Academy of Sciences of Ukraine, MAO/NASU, 27 Akademika Zabolotnoho St, 03680 Kyiv, Ukraine
[5] The Kavli Institute for Astronomy and Astrophysics at Peking University, Beijing 100871, China - Fuente
Monthly notices of the Royal Astronomical Society (Print). 2012, Vol 419, Num 1, pp 57-69, 13 p ; ref : 1 p
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Campo Científico
- Astronomy earth cosmic environment
- Editor
- Wiley-Blackwell, Malden, MA
- País de la publicación
- United States
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave de autor
- black hole physics galaxies: evolution galaxies: kinematics and dynamics galaxies: nuclei gravitation
- Palabra clave (fr)
- Cinématique Cosmologie Cône perte Dynamique Evolution galaxies Galaxies Gravitation Instabilité gravitationnelle Instabilité séculaire Noyau galaxies Sphère Symétrie sphérique Temps relaxation Trou noir Voie lactée
- Palabra clave (in)
- Kinematics Cosmology Loss cone Dynamics Galaxy evolution Galaxies Gravitation Gravitational instability Secular instability Galaxy nuclei Spheres Spherical symmetry Relaxation time Black holes Milky Way
- Palabra clave (es)
- Evolución galaxias Inestabilidad secular Simetría esférica
- Clasificación
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 25289677
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
10.1111/j.1365-2966.2011.19670.x 
https://dx.doi.org/10.1111/j.1365-2966.2011.19670.x
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