An RXTE observation of MCG-6-30-15: constraints on the iron abundance and reflective fraction relationship

Details An RXTE observation of MCG-6-30-15: constraints on the iron abundance and reflective fraction relationship An RXTE observation of MCG-6-30-15: constraints on the iron abundance and reflective fraction relationship

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999nuphs..69..486l&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 69, Issue 1-3, p. 486-489.

Physics

Nuclear Physics

Scientific paper

We report on a 50ks observation of the bright Seyfert 1 galaxy MCG-6-30-15 with the Rossi X-ray Timing Explorer. The data clearly show the broad fluorescent iron line (equivalent width ~242eV for the scenario in which the primary X-ray source is above the accretion disk subtending an angle of 2π sr), and the Compton reflection continuum at higher energies. Upper limit constraints on the abundance versus reflective fraction relationship can already be placed at the 68 per cent confidence level.

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