2014/03/07 by Lucas Labadie, Labadie, Lucas, Jens Zuther +9
Physics and Astronomy · #Astrophysics of Galaxies (astro-ph.GA) #FOS: Physical sciences #Instrumentation and Methods for Astrophysics (astro-ph.IM) #astro-ph.GA #astro-ph.IM
paper · pdf · doi:10.48550/arxiv.1403.1744
Proceedings of the Conference "Nuclei of Seyfert galaxies and QSOs - Central engine & conditions of star formation" (Bonn, Germany, 6-8 November 2012)
arxiv created 2014/03/11 · arxiv updated 2014/03/13
We explore the scientific potential of next-generation high-angular resolution optical imager to study the AGN/Host connection. The availability of a significant number of X-raying AGN with natural guide stars, allowing for adaptive optics at optical wavelengths, offers an interesting perspective to complement high-resolution work currently done in the near-infrared.