Figure 19 from Mid-infrared Outbursts in Nearby Galaxies (MIRONG). I. Sample Selection and Characterization

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Mid-infrared Outbursts in Nearby Galaxies (MIRONG). I. Sample Selection and Characterization

Authors: Ning Jiang, Tinggui Wang, Liming Dou, Xinwen Shu, Xueyang Hu, Hui Liu, Yibo Wang, Lin Yan, Zhenfeng Sheng, Chenwei Yang, Luming Sun, and Hongyan Zhou

2021 The Astrophysical Journal Supplement Series 252 32.

Provider: AAS Journals

Caption: Figure 19.

Left panel: correlation between peak MIR luminosity (L_d) and M_BH. Right panel: correlation between inferred dust mass (M_d) and M_BH. Overlaid in red is the linear least-squares fitting. The L_d and M_d values are derived by dust with absorption efficiency (see Table 3).

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