AGN coronal emission models – I. The predicted radio emission
نویسندگان
چکیده
منابع مشابه
Coronal Heating and Emission Mechanisms in Agn
Popular models for the formation of X-ray spectra in AGN assume that a large fraction of the disk’s angular momentum dissipation takes place in a hot corona that carries a small amount of the accreting mass. Here I discuss the formation of a magnetically–structured accretion disk corona, generated by buoyancy instability in the disk and the heating of localized flare regions up to the canonical...
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Using the most recent (April 2003) version of the VLA FIRST survey radio catalog, we have searched for radio emission from > 2800 AGN taken from the most recent (2001) version of the Veron-Cetty and Veron AGN catalog. These AGN lie in the ∼9033 square degrees of sky already covered by the VLA FIRST survey. Our work has resulted in positive detection of radio emission from 775 AGN of which 214 a...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2016
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/stw772