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Catalog Service:
11.5um image of NGC 835

Short name: J/A+A/587/A1
IVOA Identifier: ivo://CDS.VizieR/J/A+A/587/A1
DOI (Digital Object Identifier): 10.26093/cds/vizier.35870001
Publisher: CDS[+][Pub. ID]
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/587/A1
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2016 Feb 11 08:51:50Z
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Description


Obscured active galactic nuclei (AGNs) are thought to be very common in the Universe. Observations and surveys have shown that the number of sources increases for near galaxies and at the low-luminosity regime (the so-called LLAGNs). Furthermore, many AGNs show changes in their obscuration properties at X-rays that may suggest a configuration of clouds very close to the accretion disk. However, these variations could also be due to changes in the intrinsic continuum of the source. It is therefore important to study nearby AGN to better understand the locus and distribution of clouds in the neighbourhood of the nucleus. We aim to study the nuclear obscuration of LLAGN NGC 835 and its extended emission using mid-infrared observations. We present sub-arcsecond-resolution mid-infrared 11.5um imaging of the LLAGN galaxy NGC 835 obtained with the instrument CanariCam in the Gran Telescopio CANARIAS (GTC), archival Spitzer/IRS spectroscopy, and archival Chandra data observed in 2000, 2008, and 2013.

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under Cooperative Agreement AST0122449 with the Johns Hopkins University
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