Figure 4 from SUPERMASSIVE BLACK HOLES WITH HIGH ACCRETION RATES IN ACTIVE GALACTIC NUCLEI. VI. VELOCITY-RESOLVED REVERBERATION MAPPING OF THE Hβ LINE

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

SUPERMASSIVE BLACK HOLES WITH HIGH ACCRETION RATES IN ACTIVE GALACTIC NUCLEI. VI. VELOCITY-RESOLVED REVERBERATION MAPPING OF THE Hβ LINE

Authors: Pu Du, Kai-Xing Lu, Chen Hu, Jie Qiu, Yan-Rong Li, Ying-Ke Huang, Fang Wang, Jin-Ming Bai, Wei-Hao Bian, Ye-Fei Yuan, Luis C. Ho, and Jian-Min Wang

2016 The Astrophysical Journal 820 27.

Provider: AAS Journals

Caption: Figure 4.

Artificial AGN spectrum in the Monte Carlo simulation. The black line is the created artificial AGN spectrum. The components are: (a) a power-law continuum (blue), (b) Fe II emission (green) and broad He II (purple), (c) narrow emission lines of [O III]λλ4959, 5007 (orange), and (d) a broad component of Hβ (red).

Other Images in This Article

Copyright and Terms & Conditions