Compton Thick AGN in the Suzaku Era(Chapter 10. Super Massive Black Holes, The Extreme Universe in the Suzaku Era)

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概要

• 論文の詳細を見る

• Suzaku observations of two hard X-ray (>10keV) selected nearby Seyfert 2 galaxies are presented. Both sources were clearly detected with the pin Hard X-ray Detector up to several tens of keV, allowing for a fairly good characterization of the broad band X-ray continuum. Both sources are heavily obscured, one of which (NGC 5728) being Compton thick, while at lower energies the shape and intensity of the scattered/reflected continuum is very different. Strong iron Kα lines are detected in both sources. There are also hints for the presence of a broad relativistic iron line in NGC 4992.

• 2007-12-19

著者

• GILLI Roberto

  INAF-Osservatorio Astronomico di Bologna

• COMASTRI Andrea

  INAF-Osservatorio Astronomico di Bologna

• VIGNALI Cristian

  Dipartimento di Astronomia, Universita degli Studi di Bologna

• Iwasawa Kazushi

  Mpe-garching

• MATT Giorgio

  Dipartimento di Fisica, Universita di Roma Tre

• FIORE Fabrizio

  INAF-Osservatorio Astronomico di Roma

• Matt Giorgio

  Dipartimento Di Fisica Universita Di Roma Tre

• Matt Giorgio

  Dipartimento Di Fisica Universita Degli Studi "roma Tre

• Vignali Cristian

  Dipartimento Di Astronomia Universita Di Bologna

関連論文

• Compton-Thick AGN and the Synthesis of the Cosmic X-Ray Background : The Suzaku Perspective(Chapter 10. Super Massive Black Holes, The Extreme Universe in the Suzaku Era)
• Compton Thick AGN in the Suzaku Era(Chapter 10. Super Massive Black Holes, The Extreme Universe in the Suzaku Era)
• Relativistic Iron Features from X-Ray Illuminated Spots and the Measure of the Black Hole Mass in AGN(Poster)
• Relativistic Iron Features from X-Ray Illuminated Spots and the Measure of the Black Hole Mass in AGN(Poster)

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