Searching for X-ray Flares from the Nucleus of M32

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Chandra Proposal Id #06700538

Scientific paper

The massive Black Hole at the center of our galaxy shows remarkable short timescale X-ray flaring that has not been detected in any other system. We propose a deep 125 ksec observation of the nucleus of M32 to search for analogous X-ray flares. We argue that the black hole mass and luminosity of M32 make it the most promising known system, other than the Galactic Center, for searching for such flaring. The detection of X-ray flaring in a second system would provide powerful new constraints on this remarkable phenomena.

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