English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
Add to Basket
  Local TagsRelease HistoryDetailsSummary

Released
Journal Article

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

MPS-Authors
/persons/resource/persons26290

Zhang,  Xue-Guang
Cosmology, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons4706

Kauffmann,  Guinevere
Cosmology, MPI for Astrophysics, Max Planck Society;

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)
There are no public fulltexts stored in PuRe
Supplementary Material (public)
There is no public supplementary material available
Citation

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.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-A228-7
Abstract
There is no abstract available