NGC1068 MIDI/VLTI observations Virtual Observatory Resource

Authors

1. Lopez-Gonzaga N.
2. Jaffe W.
3. Burtscher L.
4. Tristram K.R.W.
5. Meisenheimer K.

Published by

CDS

Abstract

The aim of this paper is to understand the relation in active galactic nuclei (AGNs) between the small obscuring torus and dusty structures at larger scales (5-10pc). The dusty structures in AGNs are best observed in the mid-infrared. To achieve the necessary spatial resolution (20-100 milliarcsec) we use ESO's Mid-Infrared Interferometer (MIDI) with the 1.8m Auxiliary Telescopes. We use the chromatic phases in the data to improve the spatial fidelity of the analysis.

Keywords

1. active-galactic-nuclei
2. interferometry

Bibliographic source Bibcode

2014A&A...565A..71L

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/565/A71

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/565/A71

Document Object Identifer DOI

doi:10.26093/cds/vizier.35650071

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