Partial dust obscuration in active galactic nuclei as a cause of broad-line profile and lag variability, and apparent accretion disc inhomogeneities

Gaskell, C. Martin; Harrington, P Z

doi:10.1093/mnras/sty848

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Partial dust obscuration in active galactic nuclei as a cause of broad-line profile and lag variability, and apparent accretion disc inhomogeneities

Author(s): C Martin Gaskell ¹ , P Z Harrington ¹

Publication date Created: April 04 2018

Publication date (Electronic): April 04 2018

Journal: Monthly Notices of the Royal Astronomical Society

Publisher: Oxford University Press (OUP)

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Title: Monthly Notices of the Royal Astronomical Society

Publisher: Oxford University Press (OUP)

ISSN (Print): 0035-8711

ISSN (Electronic): 1365-2966

Publication date Created: August 2018

Publication date Created: August 01 2018

Publication date Created: April 04 2018

Publication date Other: August 2018

Publication date (Print): August 01 2018

Publication date (Electronic): April 04 2018

Volume: 478

Issue: 2

Pages: 1660-1669

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[1 ]Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA

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DOI: 10.1093/mnras/sty848

SO-VID: 8d7374b3-db63-4476-994c-1f29247a2289

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Partial dust obscuration in active galactic nuclei as a cause of broad-line profile and lag variability, and apparent accretion disc inhomogeneities

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