Figure 6 from Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. VIII. Structure of the Broad-line Region and Mass of the Central Black Hole in Mrk 142

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Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. VIII. Structure of the Broad-line Region and Mass of the Central Black Hole in Mrk 142

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

2018 The Astrophysical Journal 869 137.

Provider: AAS Journals

Caption: Figure 6.

Examples of inferred geometry of the BLR for the three models from top to bottom. Each point represents a BLR particle and its size is in proportion to the weight of emissivity in Equation (15). For model M3, red and blue points correspond to BLR particles from zone I and zone II, respectively.

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