X-ray spectroscopy of a recoiling SMBH candidate

Details X-ray spectroscopy of a recoiling SMBH candidate X-ray spectroscopy of a recoiling SMBH candidate

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cxo..prop.2728p&link_type=abstract

Chandra proposal ID #10700034

Physics

Scientific paper

Recent numerical relativity simulations of coalescencing supermassive black hole (SMBH) binaries predict that SMBHs can receive kicks with velocities up to several thousand km/s due to anisotropic emission of gravitational waves. We have recently found the best candidate todate for such a recoiling SMBH (Komossa et al. 2008). We apply for a 25 ks ACIS-S exposure of this exceptional source.

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