HCN TO HCO+ MILLIMETER LINE DIAGNOSTICS OF AGN MOLECULAR TORI. I. RADIATIVE TRANSFER MODELING
- Author
- YAMADA, Masako1 ; WADA, Keiichi2 ; TOMISAKA, Kohji2
[1] ALMA Project Office, National Astronomical Observatory of Japan, Mitaka, Osawa 181-8588, Japan
[2] Division of Theoretical Astronomy, National Astronomical Observatory of Japan, Mitaka, Osawa 181-8588, Japan - Source
The Astrophysical journal. 2007, Vol 671, Num 1, pp 73-84, 12 p ; 1 ; ref : 1/2 p
- 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: molecules galaxies: ISM galaxies: active radiative transfer radio lines: galaxies
- Keyword (fr)
- Cyanure d'hydrogène Galaxies actives Modélisation Noyau galactique actif Noyau galaxies Radiogalaxies Radiosource cosmique Tore Transfert radiatif
- Keyword (en)
- Hydrogen cyanides Active galaxies Modelling Active galaxy nuclei Galaxy nuclei Radio galaxies Cosmic radio sources Tori Radiative transfer
- Keyword (es)
- Hidrogeno cianuro
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 19924432
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
10.1086/522332 
https://dx.doi.org/10.1086/522332
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