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A Possible Detection of M31* with Chandra

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© 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Michael R. Garcia et al 2005 ApJ 632 1042 DOI 10.1086/432967

0004-637X/632/2/1042

Abstract

Two independent sets of Chandra and HST images of the nuclear region of M31 allow registration of X-ray and optical images to ~0farcs1. This registration shows that none of the bright (~1037 ergs s-1) X-ray sources near the nucleus is coincident with the central supermassive black hole, M31*. A 50 ks Chandra HRC image shows 2.5 σ evidence for a faint (~1036 ergs s-1) discrete source that is consistent with the position of M31*. The Bondi radius of M31* is 0farcs9, making it one of the few supermassive black holes with a resolvable accretion flow. This large radius and the previous detections of diffuse X-ray-emitting gas in the nuclear region make M31* one of the most secure cases for a radiatively inefficient accretion flow and place some of the most severe constraints on the radiative processes in such a flow.

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10.1086/432967