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Astronomy & Astrophysics 541 (2012) L9
VLTI/AMBER observations of the Seyfert nucleus of NGC 3783
G. Weigelt 1, K.-H. Hofmann 2, M. Kishimoto 3, S. Hönig 4, D. Schertl 3, A. Marconi 5, F. Millour 6, R. Petrov 6, D. Fraix-Burnet 7, F. Malbet 7, K. Tristram 3, M. Vannier 6
(2012-05)

Context. The putative tori surrounding the accretion disks of active galactic nuclei (AGNs) play a fundamental role in the unification scheme of AGNs. Infrared long-baseline interferometry allows us to study the inner dust distribution in AGNs with unprecedented spatial resolution over a wide infrared wavelength range. Aims: Near- and mid-infrared interferometry is used to investigate the milli-arcsecond-scale dust distribution in the type 1.5 Seyfert nucleus of NGC 3783. Methods: We observed NGC 3783 with the VLTI/AMBER instrument in the K-band and compared our observations with models. Results: From the K-band observations, we derive a ring-fit torus radius of 0.74 ± 0.23 mas or 0.16 ± 0.05 pc. We compare this size with infrared interferometric observations of other AGNs and UV/optical-infrared reverberation measurements. For the interpretation of our observations, we simultaneously model our near- and mid-infrared visibilities and the spectral energy distribution (SED) with a temperature/density-gradient model including an additional inner hot 1400 K ring component. Based on observations made with ESO telescopes at Paranal Observatory under programme IDs 083.B-0212(A) and 087.B-0578(A).
1:  Max Planck Institute Für RadioAstronomie (MPIFR)
Max-Planck-Institut
2:  Max-Planck Institut für Radioastronomie (MPIFR)
Max-Planck-Institut
3:  Max-Planck-Institut für Radioastronomie (MPIFR)
Max-Planck-Institut
4:  UCSB Department of Physics (UCSB)
UCSB
5:  Osservatorio Astrofisico di Arcetri (OAA)
Istituto Nazionale di Astrofisica
6:  Joseph Louis LAGRANGE (LAGRANGE)
Observatoire de la Côte d'Azur – Université Nice Sophia Antipolis [UNS] – CNRS : UMR7293
7:  Institut de Planétologie et d'Astrophysique de Grenoble (IPAG)
CNRS : UMR5274 – INSU – Université Joseph Fourier - Grenoble I – OSUG
Sciences of the Universe/Astrophysics/Galactic Astrophysics

Physics/Astrophysics/Galactic Astrophysics
galaxies: active – galaxies: Seyfert – techniques: interferometric – galaxies: individual: NGC 3783
Fulltext link: 
http://fr.arXiv.org/abs/1204.6122