Tidally disrupted dusty clumps as the origin of broad emission lines in active galactic nuclei-Reference-Cited by-同舟云学术

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Tidally disrupted dusty clumps as the origin of broad emission lines in active galactic nuclei

Published:2017-10-09 Issue:11 Volume:1 Page:775-783
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Wang Jian-Min,Du Pu,Brotherton Michael S.,Hu Chen,Songsheng Yu-Yang,Li Yan-Rong,Shi Yong,Zhang Zhi-Xiang

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://www.nature.com/articles/s41550-017-0264-4.pdf

Reference110 articles.

1. Ho, L. C. Nuclear activity in nearby galaxies. Annu. Rev. Astron. Astrophys. 46, 475–539 (2008).

2. Gaskell, C. M. What broad emission lines tell us about how active galactic nuclei work. New Astron. Rev. 53, 140–148 (2009).

3. Korista, K. What’s emitting the broad emission lines? ASP Conf. Series 162, 165–176 (1999).

4. Antonucci, R. R. J. Unified models for active galactic nuclei and quasars. Annu. Rev. Astron. Astrophys. 31, 473–521 (1993).

5. Jaffe, W. et al. The central dusty torus in the active nucleus of NGC 1068. Nature 429, 47–49 (2004).

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