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    The lack of torus emission from BL Lacertae objects: An infrared view of unification with WISE

    251723.pdf (716.9Kb)
    Access Status
    Open access
    Authors
    Plotkin, Richard
    Anderson, S.
    Brandt, W.
    Markoff, S.
    Shemmer, O.
    Wu, J.
    Date
    2012
    Type
    Journal Article
    
    Metadata
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    Citation
    Plotkin, R. and Anderson, S. and Brandt, W. and Markoff, S. and Shemmer, O. and Wu, J. 2012. The lack of torus emission from BL Lacertae objects: An infrared view of unification with WISE. Astrophysical Journal Letters. 745: L27.
    Source Title
    Astrophysical Journal Letters
    DOI
    10.1088/2041-8205/745/2/L27
    ISSN
    2041-8205
    School
    Department of Physics and Astronomy
    Remarks

    Copyright © 2012 The American Astronomical Society. All rights reserved..

    URI
    http://hdl.handle.net/20.500.11937/52853
    Collection
    • Curtin Research Publications
    Abstract

    We use data from the Wide-Field Infrared Survey Explorer (WISE) to perform a statistical study on the mid-infrared (IR) properties of a large number (102) of BL Lac objects - low-luminosity active galactic nuclei (AGNs) with a jet beamed toward the Earth. As expected, many BL Lac objects are so highly beamed that their jet synchrotron emission dominates their IR spectral energy distributions. In other BL Lac objects, however, the jet is not strong enough to completely dilute the rest of the AGN emission. We do not see observational signatures of the dusty torus from these weakly beamed BL Lac objects. The lack of observable torus emission is consistent with suggestions that BL Lac objects are fed by radiatively inefficient accretion disks. Implications for the "nature versus nurture" debate for FR I and FR II radio galaxies are briefly discussed. Our study supports the notion that, beyond orientation, accretion rate plays an important role in AGN unification.

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