Probing the dusty environment of the Seyfert 1 nucleus in NGC 3783 with MIDI/VLTI interferometry

Astronomy and Astrophysics

Volumn 486, Issue 3, 2008, Pages

  Beckert, T ^a   Driebe, T ^a   Honig, S F ^a   Weigelt, G ^a  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

Author keywords

Galaxies: active; Galaxies: individual: NGC 3783; Galaxies: nuclei; Galaxies: Seyfert; Techniques: interferometric radiation mechanisms: thermal

Indexed keywords

DISKS (STRUCTURAL COMPONENTS); EMISSION SPECTROSCOPY; GEODETIC SATELLITES; IMAGING TECHNIQUES; INTERFEROMETERS; INTERFEROMETRY; LAWS AND LEGISLATION; LUMINANCE; OPTICAL INSTRUMENTS; OPTICAL PROPERTIES; OPTICAL TELESCOPES; PHOTOGRAPHY; SILICATES; TELESCOPES; VISIBILITY;

BAND SPECTRUM; BOLOMETRIC LUMINOSITIES; CROSS SECTIONAL INFRARED (IR) OBSERVATIONS; DISK MODEL; DUST CLOUDS; DUST ENVIRONMENT; IR EMISSIONS; MONOTONIC INCREASE; OPTICAL (PET) (OPET); SEYFERT (CO); SPATIALLY RESOLVED; SPECTRA (CO); VERY LARGE TELESCOPE INTERFEROMETER (VLTI); WAVELENGTH DEPENDENCE; WAVELENGTH RANGES; X RAY OBSERVATIONS;

DUST;

EID: 47749118307     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078881     Document Type: Article

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