Hostname: page-component-745bb68f8f-s22k5 Total loading time: 0 Render date: 2025-01-13T11:09:28.880Z Has data issue: false hasContentIssue false
  • English
  • Français

Clumpy Scattering Regions in Active Galactic Nuclei

Published online by Cambridge University Press:  12 April 2016

Makoto Kishimoto
Makoto Kishimoto*
Affiliation:
Department of Astronomy, Faculty of Science, Kyoto University, Kyoto 606-01, Japan

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Simple unified models predict that many Seyfert 2s should be highly polarized ( ≳ 50%), but such highly polarized Seyfert 2s are not observed. As one of the possibilities to explain this problem, the existence of clumpy scattering clouds with optically thick condensations in the nuclear regions is discussed.

Type
X. Unification of Active Galaxies and Other Global Issues
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 457 - 458
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Antonucci, R., Hurt, T., & Miller, J.S. 1994, ApJ, 430, 210.Google Scholar
Kishimoto, M. 1996, ApJ, 468, 606.CrossRefGoogle Scholar
Miller, J.S., & Goodrich, R.W. 1990, ApJ, 355, 456.CrossRefGoogle Scholar
Tran, H.D. 1995, ApJ, 440, 565.CrossRefGoogle Scholar