Ionized gas within roughly 600 pc of the supermassive black hole in PKS 0745-191 is chaotic and non-rotating, with a sharp central velocity dispersion that suggests a black hole of about 1.5e10 solar masses.
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HST Observations within the Sphere of Influence of the Powerful Supermassive Black Hole in PKS0745-191
Ionized gas within roughly 600 pc of the supermassive black hole in PKS 0745-191 is chaotic and non-rotating, with a sharp central velocity dispersion that suggests a black hole of about 1.5e10 solar masses.