Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/18817
Title: Clumpy stellar winds and the obscuration of active galactic nuclei
Authors: Nayakshin, S.
Cuadra, J.
First Published: Apr-2007
Publisher: EDP Sciences for European Southern Observatory (ESO)
Citation: Astronomy & Astrophysics, 2007, 465 (1), pp. 119-124
Abstract: The role of star-formation driven outflows in the obscuration of the central source in Active Galactic Nuclei (AGN) is discussed. The outflow from a sub-parsec scale accretion disc is numerically modelled for parameters appropriate to the Galactic Centre. The resulting obscuration pattern is very patchy, with some lines of sight becoming optically thick to Thomson scattering. A fixed observer would see column depth changing by factors of many over time scales ranging from months to hundreds of years, depending on the physical size of the outflow region. Such winds may be relevant for the obscuration of some AGN, especially "changing look AGN". The winds are Thomson-thick for outflow rates exceeding the Eddington accretion rate limit, which may be satisfied in strong near-AGN starbursts as observed in a few nearby galactic nuclei.
DOI Link: 10.1051/0004-6361:20065541
ISSN: 0004-6361
eISSN: 1432-0746
Links: http://hdl.handle.net/2381/18817
http://www.aanda.org/articles/aa/abs/2007/13/aa5541-06/aa5541-06.html
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2007 ESO. Reproduced with permission from Astronomy & Astrophysics, © ESO.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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