... Our group has been studying the co-evolution of AGN, BHs, and their host galaxies for several years now. ... We rely on a multiwavelength approach, from the millimeter and the IR to the X-ray. ...
... LIMITS ON THE ROTATION OF UV LINEAR POLARIZATION OF RADIO GALAXIES AT z > 2 UV (at 1300 ° restframe), and with elongated optiA, cal morphology at these wavelengths, since these are the marking characteristics of the presence of scattered nuclear ...
... Research . Adaptive Optics . Galaxies, AGN, Cosmology . High energy . Infrared astronomy . Optical turbulence . ... automated barrier just behind the gate is close, ask the guard man or ring the bell to ask for it to be opened, then proceed by ...
... Research . Adaptive Optics . Galaxies, AGN, Cosmology . High energy . Infrared astronomy . Optical turbulence . ... x=70(78B/B), DUS=80(88B/B), xx=105(121B/B) . Notes: ring up hotel when back later than 01.00 am . ...
... galaxies from the two samples are also highlighted in future plots to separate them ... MAGPHYS rest-frame SED fit to H-ATLAS elliptical galaxy 298980. ... MAGPHYS rest-frame SED fit to HeViCS elliptical galaxy VCC 408. ...
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Ссылки http://www.arcetri.astro.it/~sperello/2015MNRAS451_3815.pdf -- 2633.2 Кб -- 20.07.2015 Похожие документы
... Adaptive Optics . Galaxies, AGN, Cosmology . High energy . Infrared astronomy . ... is a general consensus that every single massive galaxy hosts a central black hole ...
... Research . Adaptive Optics . Galaxies, AGN, Cosmology . High energy . Infrared astronomy . Optical turbulence . ... in the Ks band by Garu fi et al. (2014 ), who saw a ring in the polarized diff erential images centered at a radius of 100 AU ...
... cloud M in the North-Western side of the Virgo cluster (Ftaclas, Fanelli & Struble 1984), where the X-ray surface brightness is low (BЖhringer et al. 1994) and spiral galaxies appear to be less HI-deficient than in the rest of the cluster (Gavazzi et al ...
... Previous modeling of the rest-frame ultraviolet emission from the extended narrow-line region of the radio galaxy has shown that it is powered predominantly by illumination by the central AGN (V01; Humphrey et al. 2008b). ...