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X-ray Studies of the Central Engine in Active Galactic Nuclei with Suzaku [[electronic resource] /] / by Hirofumi Noda



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Autore: Noda Hirofumi Visualizza persona
Titolo: X-ray Studies of the Central Engine in Active Galactic Nuclei with Suzaku [[electronic resource] /] / by Hirofumi Noda Visualizza cluster
Pubblicazione: Singapore : , : Springer Singapore : , : Imprint : Springer, , 2016
Edizione: 1st ed. 2016.
Descrizione fisica: 1 online resource (164 p.)
Disciplina: 523.112
Soggetto topico: Observations, Astronomical
Astronomy - Observations
Physical measurements
Measurement   
Astronomy, Observations and Techniques
Measurement Science and Instrumentation
Note generali: "Doctoral thesis accepted by the University of Tokyo, Tokyo, Japan."
Nota di bibliografia: Includes bibliographical references at the end of each chapters.
Nota di contenuto: Review -- Instrumentation -- Observation and Data Reduction -- Soft X-ray Analysis -- Hard X-ray Analysis -- Discussion and Conclusion.
Sommario/riassunto: 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.
Titolo autorizzato: X-ray Studies of the Central Engine in Active Galactic Nuclei with Suzaku  Visualizza cluster
ISBN: 981-287-721-5
Formato: Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione: Inglese
Record Nr.: 9910254609303321
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Serie: Springer Theses, Recognizing Outstanding Ph.D. Research, . 2190-5053