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We point out that the tidal disruption of a giant may leave a luminous(10^35-10^39 ergs/s), hot (10-100 eV) stellar core. The ``supersoft'' sourcedetected by Chandra at the center of M31 may be such a core; whether or not itis, the observations have shown that such a core is detectable, even in thecenter of a galaxy. We therefore explore the range of expected observationalsignatures and how they may be used to (1) test the hypothesis that the M31source is a remnant of tidal stripping and (2) discover evidence of black holesand disruption events in other galaxies.Comment: Four pages with 1 figure. Appeared in ApJL (2001, 551, L37

A New Way to Detect Massive Black Holes in Galaxies: The Stellar Remnants of Tidal Disruption