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X-ray Studies of the Central Engine in Active Galactic Nuclei with Suzaku

  • Book
  • © 2016

Overview

  • Nominated as an outstanding contribution by The University of Tokyo's Department of Astronomy in 2013
  • Presents a technique for variability-assisted spectral decomposition of X-ray components generated in an active galactic nucleus
  • Proposes a novel picture of the central engine, formed by multiple coronae and an accretion disk onto a supermassive black hole, in an active galactic nucleus
  • Includes supplementary material: sn.pub/extras

Part of the book series: Springer Theses (Springer Theses)

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Table of contents (6 chapters)

Keywords

About this book

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.

Authors and Affiliations

  • Department of Astronomy, School of Science, The University of Tokyo, Tokyo, Japan

    Hirofumi Noda

About the author

Dr. Hirofumi Noda

Department of Astronomy, The University of Tokyo


Bibliographic Information

  • Book Title: X-ray Studies of the Central Engine in Active Galactic Nuclei with Suzaku

  • Authors: Hirofumi Noda

  • Series Title: Springer Theses

  • DOI: https://doi.org/10.1007/978-981-287-721-5

  • Publisher: Springer Singapore

  • eBook Packages: Physics and Astronomy, Physics and Astronomy (R0)

  • Copyright Information: Springer Science+Business Media Singapore 2016

  • Hardcover ISBN: 978-981-287-720-8Published: 15 December 2015

  • Softcover ISBN: 978-981-13-5708-4Published: 09 December 2018

  • eBook ISBN: 978-981-287-721-5Published: 07 December 2015

  • Series ISSN: 2190-5053

  • Series E-ISSN: 2190-5061

  • Edition Number: 1

  • Number of Pages: XV, 153

  • Number of Illustrations: 62 b/w illustrations, 33 illustrations in colour

  • Topics: Astronomy, Observations and Techniques, Measurement Science and Instrumentation

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