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3.28. Three-dimensional distribution of the nuclear mirrors in NGC 1068

Published online by Cambridge University Press:  25 May 2016

Makoto Kishimoto
Makoto Kishimoto*
Affiliation:
Kyoto University Sakyo-ku, Kyoto 606-01, Japan

Extract

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Recently, the HST imaging observations have revealed that the central arc second region in NGC 1068 has a clumpy structure (Macchetto et al., 1994) and the HST UV imaging polarimetry has revealed the centrosymmetric pattern of the position angles of polarization (Capetti et al., 1995), which indicates that the medium in this region is actually scattering the radiation from a small source, in accordance with the unified model of active galactic nuclei (Antonucci & Miller, 1985).

Type
Part I. Stellar Cluster, Star Formation
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 145 - 146
Copyright
Copyright © Kluwer 1998 

References

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