... galactic light (DGL) and in recent years galaxies and active galactic nuclei (AGN ... SED . late type stars, AGN . Hoefflich [ 1991 ] . MC . Thomson scattering . ... 2D (homogeneous torus) . SED . AGN, Seyfert galaxies . Bosma [ 1993a ], [ 1993b ] . ...
... Task 5 (Astrophysical applications) The radiation transfer codes developed in Jena have been applied to different cosmic objects, for instance: AGN by Wolf & Henning ("AGN polarization models." ...
... polarisation at 35 m, produced by emission from hot dust located close to the AGN ... regions to be viewed (e.g. in an AGN or young star, radiation can escape along the ... the processes of accretion, disk formation and mass out ow, for stars and AGN ...
... Groningen, Netherlands) "Simulating the Universes Epoch of Reionization" 16.30 17.00 Sergei Komissarov, O. Porth (Univ. of Leeds, UK) "Stability of AGN jets and the Fanaroff-Riley division" 17.00 17.30 Coffee break 17.30 18.00 Nikolai Shakura, K.A ...
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Ссылки http://www.astro.spbu.ru/Sobolev100/sites/default/files/ProgramFinal_0.pdf -- 313.0 Кб -- 28.09.2015 Похожие документы
... S. Komissarov, O. Porth Stability of AGN jets and the Fanaroff-Riley division . ... of the broad emission line region (BLR) in Active Galactic Nuclei (AGN) are unclear ... new estimates of SMBH masses in AGN with measured polarization of broad lines ...
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Ссылки http://www.astro.spbu.ru/Sobolev100/sites/default/files/Sobolev-100.pdf -- 2775.2 Кб -- 02.10.2015 Похожие документы
... For applications to circumbinary disks, warped disks, disks with planets, and AGN dust tori, as well for a 3D benchmark test including images, we refer to the later papers of this series. ...