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

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Published 2001 March 27 © 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation R. Di Stefano et al 2001 ApJ 551 L37 DOI 10.1086/319835

1538-4357/551/1/L37

Abstract

We point out that the tidal disruption of a giant may leave a luminous (1035-1039 ergs s-1), hot (10-100 eV) stellar core. The "supersoft" source detected by Chandra at the center of M31 may be such a core; whether or not it is, the observations have shown that such a core is detectable, even in the center of a galaxy. We therefore explore the range of expected observational signatures and how they may be used to (1) test the hypothesis that the M31 source is a remnant of tidal stripping and (2) discover evidence of black holes and disruption events in other galaxies.

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10.1086/319835