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X-ray Studies of the Central Engine in Active Galactic Nuclei with Suzaku (Hardcover, 1st ed. 2016)
Loot Price: R2,832
Discovery Miles 28 320
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X-ray Studies of the Central Engine in Active Galactic Nuclei with Suzaku (Hardcover, 1st ed. 2016)
Series: Springer Theses
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The aim of this research was to use the X-ray satellite Suzaku to
establish a picture of a central engine that effectively converts
the gravitational energy of accreting matter onto the supermassive
black hole to a huge amount of radiation in an active galactic
nucleus. Although the engine is known to consist of a Comptonizing
corona and an accretion disk, its image has remained unclear
because primary emissions, coming directly from the engine, cannot
be identified in X-ray spectra without models. The book describes a
technique of time variability assisted spectral decomposition to
model-independently examine X-ray signals, and how this was applied
to the Suzaku archive data of active galactic nuclei. As a result,
at least three distinct primary X-ray components have been
discovered in an X-ray from an active galactic nucleus, presumably
indicating a novel picture that the engine is composed of multiple
coronae with different physical properties in an accretion flow.
Furthermore, the determination of the spectral shapes of the
primary X-rays has a significant impact on estimations of black
hole spins, because it is essential to quantify reprocessed X-ray
spectra. The successful model-independent decomposition of X-ray
spectral components with flux variations of active galactic nuclei
is likely to be effective in future data analyses from the
soon-to-be-launched Japanese X-ray satellite ASTRO-H, which is
capable of achieving unprecedented fine spectros copy and broad
energy band coverage.
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