Long-Term X-ray Spectral Variability in Seyfert 1 Galaxies

Details Long-Term X-ray Spectral Variability in Seyfert 1 Galaxies Long-Term X-ray Spectral Variability in Seyfert 1 Galaxies

2003-08-18

arxiv.org/abs/astro-ph/0308312v1

Astrophys.J.598:935-955,2003

Astronomy and Astrophysics

Astrophysics

Accepted for publication in ApJ. 29 pages

Scientific paper

10.1086/379103

Direct time-resolved spectral fitting has been performed on continuous RXTE monitoring of seven Seyfert 1 galaxies in order to study their broadband spectral variability and Fe K alpha variability characteristics on time scales of days to years. Variability in the Fe K alpha line is not detected in some objects but is present in others, e.g., in NGC 3516, NGC 4151 and NGC 5548 there are systematic decreases in line flux by factors of ~2-5 over 3-4 years. The Fe K alpha line varies less strongly than the broadband continuum, but, like the continuum, exhibits stronger variability towards longer time scales. Relatively less model-dependent broadband fractional variability amplitude (Fvar) spectra also show weaker line variability compared to the continuum variability. Comparable systematic long-term decreases in the line and continuum are present in NGC 5548. Overall, however, there is no evidence for correlated variability between the line and continuum, severely challenging models in which the line tracks continuum variations modified only by a light-travel time delay. Local effects such as the formation of an ionized skin at the site of line emission may be relevant. The spectral fitting and Fvar spectra both support spectral softening as continuum flux increases.

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