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Do Intermediate-mass Black Holes Exist in Globular Clusters?

  • Authors: Mou-Yuan Sun, Ya-Ling Jin, Wei-Min Gu, Tong Liu, Da-Bin Lin, and Ju-Fu Lu

Sun et al. 2013 The Astrophysical Journal 776 118.

  • Provider: AAS Journals

Caption: Figure 1.

Radio luminosity L R as a function of black hole mass M BH. The filled circles represent the 3σ upper limit of L R for each source, where the black hole masses are constrained via dynamical modelings. The dashed line represents the predicted L R as a function of M BH according to Strader et al. (2012). The dot–dashed line and the thick solid line correspond to our new results with δ = 0.1 and 0.001, respectively. The thin solid line and the dotted line represent L R estimated by the relation instead of the fundamental plane relation with and without outflows, respectively.

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