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  Partly obscured accretion disc model to explain shifted broad Balmer emission lines of active galactic nuclei

Zhang, X.-G., Dultzin, D., Wang, T.-G., & Kauffmann, G. (2009). Partly obscured accretion disc model to explain shifted broad Balmer emission lines of active galactic nuclei. Monthly Notices of the Royal Astronomical Society, 397(3), 1510-1520. doi:10.1111/j.1365-2966.2009.14986.x.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-A228-7 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-A229-5
Genre: Journal Article

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 Creators:
Zhang, Xue-Guang1, Author           
Dultzin, Deborah, Author
Wang, Ting-Gui, Author
Kauffmann, Guinevere1, Author           
Affiliations:
1Cosmology, MPI for Astrophysics, Max Planck Society, ou_159876              

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Language(s): eng - English
 Dates: 2009-08-11
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: eDoc: 434393
DOI: 10.1111/j.1365-2966.2009.14986.x
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Title: Monthly Notices of the Royal Astronomical Society
  Alternative Title : Mon. Not. Roy. Astron. Soc.
Source Genre: Journal
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Pages: - Volume / Issue: 397 (3) Sequence Number: - Start / End Page: 1510 - 1520 Identifier: ISSN: 1364-8711
ISSN: 0035-8711