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The existence of stellar cusps in dense clusters around massive black holesis a fundamental, decades-old prediction of theoretical stellar dynamics. Yet,observational evidence has been difficult to obtain. With a new, improvedanalysis of high-angular resolution images of the central parsecs of theGalactic Center, we are finally able to provide the first solid evidence forthe existence of a stellar cusp around the Milky Way's massive black hole. Theexistence of stellar cusps has a significant impact on predicted event rates ofphenomena like tidal disruptions of stars and extreme mass ratio inspirals.

The stellar cusp around the Milky Way's central black hole