XMM-Newton Proposal 03053701

Details XMM-Newton Proposal 03053701 XMM-Newton Proposal 03053701

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..171m&link_type=abstract

XMM-Newton Proposal ID #03053701

Computer Science

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Eso 198-G24, Xmm-Newton Proposal 03053701

Scientific paper

ESO 198-G24 has a peculiar Fe line complex comprising a 6.4 keV emission line with variable profile. In addition, a narrow emission line component at lower energy has also been detected in the two XMM-Newton observations (at 5.7 keV and 5.9 keV respectively). The study of the variability of the two emission features in a long XMM--Newton observation will constrain their origin and potentially provides the possibility of studying in detail the strong field regime of General Relativity. If the redshifted feature will turn out to originate in an orbiting spot, we will be able to give the first X--ray estimate of the black hole mass in ESO 198-G24, as recently done by Iwasawa et al (2004) for NGC 3516.

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