Towards a physical model of dust tori in Active Galactic Nuclei: Radiative transfer calculations for a hydrostatic torus model

Astronomy and Astrophysics

Volumn 437, Issue 3, 2005, Pages 861-881

  Schartmann, M ^a   Meisenheimer, K ^a   Camenzind, M ^b   Wolf, S ^a   Henning, Th ^a  

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^b UNIVERSITÄT HEIDELBERG   (Germany)

Author keywords

Galaxies: individual: NGC 1068; Galaxies: nuclei; Galaxies: Seyfert; ISM: dust, extinction; Radiative transfer

Indexed keywords

COMPOSITION; GALAXIES; INFRARED RADIATION; LIGHT POLARIZATION; MATHEMATICAL MODELS; MONTE CARLO METHODS; PROBLEM SOLVING; RADIATION;

GALAXIES:INDIVIDUAL:NGC 1068; GALAXIES:NUCLEI; GALAXIES:SEYFERT; ISM:DUST,EXTINCTION; RADIATIVE TRANSFER;

DUST;

EID: 21844451892     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042363     Document Type: Article

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