Modeling the optical/UV polarization while flying around the tilted outflows of NGC 1068

0389049 - ASÚ 2015 RIV GB eng C - Konferenční příspěvek (zahraniční konf.)
Marin, F. - Goosmann, R. W. - Dovčiak, Michal
Modeling the optical/UV polarization while flying around the tilted outflows of NGC 1068.
Astronomy at High Angular Resolution : The Central Kiloparsec in Galactic Nuclei. Bristol: Institute of Physics Publishing, 2012, 012065/1-012065/6. Journal of Physics Conference Series, 372. ISSN 1742-6588.
[Astronomy at High Angular Resolution - The Central Kiloparsec in Galactic Nuclei. Bad Honnef (DE), 28.08.2011-02.09.2011]
Institucionální podpora: RVO:67985815
Klíčová slova: radio galaxies * NGC-1068 * spectropolarimetry
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika

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.
Trvalý link: http://hdl.handle.net/11104/0217992