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NASA NTRS · 19860050795

Limits of X-ray variability in active galactic nuclei

Abstract

A significant correlation is demonstrataed here between the X-ray luminosity and the timescale of X-ray variability for Seyfert galaxies and quasars. This is interpreted as evidence that the emitting plasma is near the limit of being dominated by electron-positron pairs. BL Lac objects do not follow this pattern; this may be due either to relativistic beaming or to the differing importance of the pair production process.

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BibTeXRIS

Barr, P., Mushotzky, R. F.. 1986-04-03. Limits of X-ray variability in active galactic nuclei. https://ntrs.nasa.gov/citations/19860050795

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