PDS 456: An extreme accretion rate quasar?

Astronomy and Astrophysics – Astronomy

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Quasars, Infall, Accretion, And Accretion Disks, X-Ray Sources, X-Ray Bursts, Galactic Nuclei, Circumnuclear Matter, And Bulges

Scientific paper

X-ray and multi-wavelength observations of the most luminous known local (z<0.3) AGN, the recently discovered radio-quiet quasar PDS 456, are presented. The spectral energy distribution shows that PDS 456 has a bolometric luminosity of 1047 erg/s, peaking in the UV. The X-ray spectrum obtained by ASCA and RXTE shows considerable complexity. The most striking feature observed is a deep, highly-ionized, iron K edge (8.7 keV, rest-frame), originating via reprocessing from highly ionized material, possibly the inner accretion disk. PDS 456 was found to be remarkably variable for its luminosity; in one flare the X-ray flux doubled in just ~15 ksec. If confirmed this would be an unprecedented event in a high-luminosity source, with a light-crossing time corresponding to ~2RS. The implications are that either flaring occurs within the very central regions, or else that PDS 456 is a `super-Eddington' or relativistically beamed system. .

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