The effect of stellar feedback on the formation and evolution of gas and dust tori in AGN

Recently, the existence of geometrically thick dust structures in active galactic nuclei (AGN) has been directly proven with the help of interferometric methods in the mid-infrared. The observations are consistent with a two-component model made up of a geometrically thin and warm central disc, surr...

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Vydané v:	Monthly notices of the Royal Astronomical Society Ročník 393; číslo 3; s. 759 - 773
Hlavní autori:	Schartmann, M., Meisenheimer, K., Klahr, H., Camenzind, M., Wolf, S., Henning, Th
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	Oxford, UK Blackwell Publishing Ltd 01.03.2009 Wiley-Blackwell Oxford University Press
Predmet:	Astronomy Astrophysics Dust dust, extinction Earth, ocean, space Exact sciences and technology extinction galaxies: nuclei galaxies: Seyfert Gases Geometry hydrodynamics ISM: evolution radiative transfer galaxies: Seyfert hydrodynamics dust, extinction galaxies: nuclei ISM: evolution radiative transfer Young cluster Spectral energy distribution Column density Neutral hydrogen Young stars Seyfert galaxies Feedback Filaments Active galaxy nuclei Surface brightness Galaxy nuclei Radiative transfer Observables Nuclear cluster model Filamentary structure Supernovae explosion Digital simulation Mass loss Star clusters Two component model Active galaxies Tori Angular momentum Hydrodynamic model Energy losses Brightness distribution Interstellar matter
ISSN:	0035-8711, 1365-2966
On-line prístup:	Získať plný text
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