Adding the Kerr quadrupole moment to the jet precession model of M87* yields a prograde solution that matches the observed time series, supporting the no-hair theorems.
Essential Relativistic Celestial Mechanics
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The no-hair theorems at work in M87$^\ast$
Adding the Kerr quadrupole moment to the jet precession model of M87* yields a prograde solution that matches the observed time series, supporting the no-hair theorems.