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The Active Fraction of Massive Black Holes in Dwarf Galaxies

  • Authors: Fabio Pacucci, Mar Mezcua, John A. Regan

Fabio Pacucci et al 2021 The Astrophysical Journal 920 .

  • Provider: AAS Journals

Caption: Figure 5.

The incidence angle θ (in degrees) required to explain a given ratio between the observationally determined ﹩{ \mathcal R }﹩ and the predicted λ B. The black dashed vertical line indicates ﹩{\lambda }_{{\rm{B}}}={ \mathcal R }﹩. The red dashed line indicates the angle of 5° required by the current IFS data. The green dashed line shows that for any value θ ≳ 50° ﹩{\lambda }_{{\rm{B}}}\sim { \mathcal R }﹩.

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