Multiwavelength Monitoring of the Black Hole in a NGC 4472 Globular Cluster

Details Multiwavelength Monitoring of the Black Hole in a NGC 4472 Globular Cluster Multiwavelength Monitoring of the Black Hole in a NGC 4472 Globular Cluster

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008head...10.0105k&link_type=abstract

American Astronomical Society, HEAD meeting #10, #1.05

Astronomy and Astrophysics

Astronomy

Scientific paper

We report on the analysis of archival and follow-up observations of the black hole in a globular cluster recently discovered by our group. This source in the nearby elliptical galaxy NGC 4472 reveals a particularly interesting optical spectrum with strong, broad, [O III] emission. We investigate the likely physical mechanisms for this emission and the implications on the properties of the black hole source. X-ray observations of the source with ROSAT, Chandra, XMM, and Swift at various points over the last decade provide further insights into the nature of the black hole.

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