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Rapid Intermediate-mass Black Hole Formation via Runaway Mergers of Black Holes

  • Authors: Yining Sun, Long Wang

Yining Sun and Long Wang 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 7.

Density profiles as a function of radius for M50k-IMF-BH and M50k-IMF-ALL under different initial conditions with half-mass radii rh• = 0.1, 0.01, and 0.001 pc. Different colors represent different initial half-mass radii. Solid lines denote the total density profile of BHs and stars combined for M50k-IMF-ALL, while dashed lines denote the BH density profiles of M50k-IMF-ALL.

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