BBXRT and GINGA observations of the Seyfert 1 galaxy MRK 335

Physics

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Continuums, Ginga Satellite, Seyfert Galaxies, Variability, X Ray Telescopes, Broadband, Ionization, Iron, X Ray Sources, X Ray Spectra

Scientific paper

We present new X-ray observations of Mrk 335 in the 0.4-10 keV band using the broadband X-ray telescope (BBXRT) and in the 2-18 keV band with Ginga. The BBXRT data show a gradual steepening of the spectrum to softer energies. We suggest that the nuclear emission can be explained by a self-consistent pair cascade model. The Ginga data show evidence for variability in absorption, uncorrected with flux changes of the continuum source. The inconsistency between the opacity observed at the iron K edge and at softer X-ray energies implies that the absorber has an ionization state BeXV.

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