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Molecular gas structure around an active galactic nucleus with nuclear starburst: Three-dimensional non-LTE calculations of CO lines

Author
WADA, Keiichi1 ; TOMISAKA, Kohji1
[1] Department of Astronomical Science, The Graduate University for Advanced Studies, Osawa 2-21-1, Mitaka, Tokyo 181-8588, Japan
Source

The Astrophysical journal. 2005, Vol 619, Num 1, pp 93-104, 12 p ; 1 ; ref : 43 ref

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
ISM: kinematics and dynamics ISM: structure galaxies: nuclei galaxies: starburst methods: numerical
Keyword (fr)
Carbone monoxyde Cinématique Dynamique Ecart ETL Ecart équilibre thermodynamique local Galaxies à flambée Gaz moléculaire Modèle 3 dimensions Modèle hydrodynamique Méthode numérique Noyau galactique actif Noyau galaxies Structure Tore Transfert radiatif
Keyword (en)
Carbon monoxide Kinematics Dynamics Non LTE Non-LTE Starburst galaxies Molecular gas Three dimensional model Hydrodynamic model Numerical method Active galaxy nuclei Galaxy nuclei Structure Tori Radiative transfer
Keyword (es)
Desviación ETL Galaxias llamarada estelar Gas molecular Modelo 3 dimensiones Método numérico Estructura
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D54 Quasars. Active or peculiar galaxies, objects, and systems / 001E03D54C Active and peculiar galaxies (including bl lacertae objects, blazars, seyfert galaxies, markarian galaxies, active galactic nuclei)

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16525255

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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