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AGN Torus Detectability at Submillimeter Wavelengths: What to Expect from ALMA Continuum Data

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    0539876 - ASÚ 2021 RIV US eng J - Journal Article
    Pasetto, A. … Total 6 authors
    AGN Torus Detectability at Submillimeter Wavelengths: What to Expect from ALMA Continuum Data.
    Astrophysical Journal. Roč. 872, č. 1 (2019), č. článku 69. ISSN 0004-637X. E-ISSN 1538-4357
    Research Infrastructure: EU-ARC.CZ - 90067
    Keywords : active galactic nuclei * variable ultraviolet-absorption * spectral-energy-distributions
    OECD category: Astronomy (including astrophysics,space science)
    Impact factor: 5.746, year: 2019
    Method of publishing: Limited access
    https://doi.org/10.3847/1538-4357/aafa20

    We study the detectability of the emission associated with the AGN dusty structure at submillimeter wavelengths using ALMA, in a theoretical and observational way. Theoretically, we use the Clumpy models from Nenkova et al., together with the MIR to X-ray and radio fundamental plane scaling relations. We find that it is more likely to detect bigger and denser dusty tori at the highest ALMA frequency (666 GHz/450 mu m). We also find that with 1 hr at 353 GHz/850 mu m and 10 hr at 666 GHz/450 mu m we can detect, with a high detection limit, a 1 mJy torus (characteristic of bright AGNs).
    Permanent Link: http://hdl.handle.net/11104/0317573

     
     
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