Accretion around Supermassive Black Holes : The Detection of the Balmer Edge Signature from Quasars(Session 5 : Evidence for Giant Black Holes)

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概要

• 論文の詳細を見る

• The ultraviolet/optical continuum of quasars is thought to be from an accretion flow around a supermassive black hole, and it dominates the radiative output of quasars. However, the nature of this emission, often called the Big Blue Bump, has not been well understood. Robust evidence for its thermal nature would be a continuum opacity edge feature intrinsic to this component, but this has not been clearly confirmed despite the predictions by many models. We are now developing and exploiting a new method to detect the Balmer edge of hydrogen opacity. The method overcomes the major obstacle of the heavy contamination from emissions outside the nucleus by taking the polarized flux spectrum. If our interpretation of the polarized flux is correct, our data show that the Big Blue Bump emission has a Balmer edge in absorption, indicating that the emission is indeed thermal, and the emitter is optically thick.

• 理論物理学刊行会の論文
• 2004-11-15

著者

• Antonucci Robert

  Physics Department University Of California

• Blaes Omer

  Physics Department University Of California

• Kishimoto Makoto

  Institute For Astronomy University Of Edinburgh

• BOISSON Catherine

  LUTH, FRE 2462 du CNRS, associee a l'Universite Denis Diderot, Observatoire de Paris

• ANTONUCCI Robert

  Physics Department, University of California

• BLAES Omer

  Physics Department, University of California

関連論文

• Accretion around Supermassive Black Holes : The Detection of the Balmer Edge Signature from Quasars(Session 5 : Evidence for Giant Black Holes)
• Accretion around Supermassive Black Holes : The Detection of the Balmer Edge Signature from Quasars(Session 5 : Evidence for Giant Black Holes)

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