10 micrometer imaging of the nucleus of NGC 1068: The bell tolls for parsec-scale tori?

Details 10 micrometer imaging of the nucleus of NGC 1068: The bell tolls for parsec-scale tori? 10 micrometer imaging of the nucleus of NGC 1068: The bell tolls for parsec-scale tori?

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994exa.....3...61c&link_type=abstract

Experimental Astronomy, vol. 3, no. 1-4, p. 61-64

Astronomy and Astrophysics

Astronomy

1

Active Galactic Nuclei, Astronomical Models, Astronomical Spectroscopy, Infrared Astronomy, Infrared Imagery, Infrared Spectra, Infrared Spectroscopy, Molecular Clouds, Seyfert Galaxies, Imaging Techniques, Line Spectra, Toruses

Scientific paper

The potential of mid-infrared imaging, at a resolution of 0.5 sec or better, as a powerful tool in unravelling the complex environments in the vicinity of active galactic nuclei (AGN) is discussed in the light of new data on the Seyfert nucleus in NGC 1068. In particular, we examine the growing body of evidence that the extinction of the broad-line region in NGC 1068 has its origins in an extended molecular disk and is the result of obscuration at approximately 100 pc from the AGN.

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