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Modeling the optical/UV polarization while flying around the tilted outflows of NGC 1068
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SYSNO ASEP 0389049 Document Type C - Proceedings Paper (int. conf.) R&D Document Type Conference Paper Title Modeling the optical/UV polarization while flying around the tilted outflows of NGC 1068 Author(s) Marin, F. (FR)
Goosmann, R. W. (FR)
Dovčiak, Michal (ASU-R) RID, ORCIDSource Title Astronomy at High Angular Resolution : The Central Kiloparsec in Galactic Nuclei. - Bristol : Institute of Physics Publishing, 2012 - ISSN 1742-6588 Pages 012065/1-012065/6 Number of pages 6 s. Publication form Print - P Action Astronomy at High Angular Resolution - The Central Kiloparsec in Galactic Nuclei Event date 28.08.2011-02.09.2011 VEvent location Bad Honnef Country DE - Germany Event type WRD Language eng - English Country GB - United Kingdom Keywords radio galaxies ; NGC-1068 ; spectropolarimetry Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics Institutional support ASU-R - RVO:67985815 UT WOS 000307718600065 DOI 10.1088/1742-6596/372/1/012065 Annotation Recent modeling of multi-waveband spectroscopic and maser observations suggests that the ionized out ows in the nuclear region of the archetypal Seyfert-2 galaxy NGC 1068 are inclined with respect to the vertical axis of the obscuring torus. Based on this suggestion, we build a complex reprocessing model of NGC 1068 for the optical/UV band. We apply the radiative transfer code stokes to compute polarization spectra and images. While a detailed analysis of our model results is still in progress, we briefly discuss how they relate to existing polarization observations of NGC 1068. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2015
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