Dynamical model of an obscuring clumpy torus in AGNs: I. velocity and velocity dispersion maps for interpretation of ALMA observations

ABSTRACT. We have developed the dynamical model of a clumpy torus in an active galactic nucleus (AGN) and compared to recent The Atacama Large Millimeter Array

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Bibliographische Detailangaben
Hauptverfasser: Bannikova, Elena Yu (VerfasserIn) , Sergeyev, A.V. (VerfasserIn) , Akerman, N.A. (VerfasserIn) , Berczik, Peter (VerfasserIn) , Ishchenko, M.V. (VerfasserIn) , Capaccioli, M. (VerfasserIn) , Akhmetov, V.S. (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2021 February 18
In: Monthly notices of the Royal Astronomical Society
Year: 2021, Jahrgang: 503, Heft: 1, Pages: 1459-1472
ISSN:1365-2966
DOI:10.1093/mnras/stab468
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stab468
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/503/1/1459/6144603
Volltext
Verfasserangaben:E.Yu Bannikova, A.V. Sergeyev, N.A. Akerman, P.P. Berczik, M.V. Ishchenko, M. Capaccioli and V.S. Akhmetov

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