Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-24T15:43:11.780Z Has data issue: false hasContentIssue false

Frequency-Dependent Polarization in Comptonization Models for AGN

Published online by Cambridge University Press:  19 July 2016

Juri Poutanen*
Affiliation:
Observatory and Astrophysics Laboratory, P.O. Box 14, SF-00014 University of Helsinki, Finland

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.

The angular distribution and the polarization of radiation as a function of the angle and frequency for the two-phase model of accretion disks in AGN are found. The results depend strongly on the temperature of the hot corona.

Type
Poster Contributions: Polarisation
Copyright
Copyright © Kluwer 1994 

References

Bisnovatyi-Kogan, G.S. and Blinnikov, S.I.: 1977, Astron. Astrophys. 59, 111 Google Scholar
Czerny, B. and Elvis, M.: 1987, Astrophys. J. 321, 305 Google Scholar
Haardt, F. and Maraschi, L.: 1993, Astrophys. J. 413, 507 CrossRefGoogle Scholar
Haardt, F. and Matt, G.: 1993, Monthly Not. Roy. Astr. Soc. 261, 346 Google Scholar
Nagirner, D.I. and Poutanen, J.: 1993a, Astron. Astrophys. 275, 325 Google Scholar
Nagirner, D.I. and Poutanen, J.: 1993b, in: Sunyaev, R.A. (ed.) Sov. Sci. Rev. E Astrophys. and Space Phys. 9, 1 Google Scholar
Poutanen, J. and Vilhu, O.: 1993, Astron. Astrophys. 275, 337 Google Scholar
Sunyaev, R.A. and Titarchuk, L.G.: 1985, Astron. Astrophys. 143, 374 Google Scholar
Wandel, A. and Liang, E.P.: 1991, Astrophys. J. 380, 84 Google Scholar