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

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

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

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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
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