Fig. 4.
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Critical line of stability for various configurations. The vertical axis is the BH mass M• plotted against azimuthal velocity vϕ. At fixed M•, the minimum azimuthal velocity vϕ to reach such that the dynamical traction sets in is found by crossing one of the black curves, from left, to right. Four curves are plotted, each corresponding to a different value of the stellar velocity dispersion σ⋆ as indicated in the legend. The blue dot marks the estimated coordinates of the Milky Way’s BH. The red curve highlights an asymptotic trend of slop ≃ − 2 found in the limit of low vϕ.
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