Figure 15 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 15.

The BH mass (M_BH) vs. stellar mass (M_*) distribution of our sample. The red filled circles are SNe, and the blue filled circles are strong jetted sources. The histograms of M_BH and M_* are shown in the right and bottom panels. Overlaid in gray dotted and magenta dashed lines are the correlation between M_BH and bulge mass (McConnell & Ma 2013) and total stellar mass (Reines & Volonteri 2015), respectively.

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