Variability and Spectroscopy of IMBH candidate in G1

Details Variability and Spectroscopy of IMBH candidate in G1 Variability and Spectroscopy of IMBH candidate in G1

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop...18m&link_type=abstract

XMM-Newton Proposal ID #06704901

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, M31Gc J003247+3

Scientific paper

We propose a 100 kilosecond observation of the M~31 globular cluster G1. This cluster is an extremely strong candidate for containing an intermediate mass black hole -- it shows evidence for an increase gravitational potential towards its center from radial velocity measurements, as well as evidence for an accreting intermediate mass black hole in the form of X-ray and radio detections. Deep XMM observations will allow the first good X-ray spectrum of this object, and will allow us to make a crude power spectrum to determine whether it fits the predictions for the power spectrum from an intermediate mass black hole at its observed luminosity.

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