From the Circumnuclear Disk in the galactic center to thick, obscuring tori of AGNs
- Autor
- VOLLMER, B1 2 ; BECKERT, T2 ; DUSCHL, W. J2 3
[1] CDS, Observatoire astronomique de Strasbourg, UMR 7550, 11 rue de l'Université, 67000 Strasbourg, France
[2] Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
[3] Institut für Theoretische Astrophysik der Universität Heidelberg, Tiergartenstrasse 15, 69121 Heidelberg, Germany - Fuente
Astronomy and astrophysics (Berlin. Print). 2004, Vol 413, Num 3, pp 949-957, 9 p ; ref : 20 ref
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Campo Científico
- Astronomy earth cosmic environment
- Editor
- EDP Sciences, Les Ulis
- País de la publicación
- France
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave de autor
- Galaxy: center Galaxy: structure ISM: clouds ISM: structure galaxies: nuclei
- Palabra clave (fr)
- Centre galactique Dispersion vitesse Disque galactique Energie cinétique Modèle Noyau galactique actif Noyau galaxies Nuage interstellaire Système autogravitant Taux accrétion Tore Transfert moment cinétique Trou noir Voie lactée
- Palabra clave (in)
- Galactic centers Velocity dispersion Galactic disks Kinetic energy Models Active galaxy nuclei Galaxy nuclei Interstellar clouds Self-gravitating systems Accretion rate Tori Angular momentum transfer Black holes Milky Way
- Palabra clave (es)
- Dispersión velocidad Modelo Índice acreción
- 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)
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 15401554
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
10.1051/0004-6361:20034201 
https://dx.doi.org/10.1051/0004-6361:20034201
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