PI: Dominika Wylezalek, Johns Hopkins U., email@example.com
Address: Department of Physics and Astronomy, Charles and 34th Street, Bloomberg Center, Baltimore, MD, 21218 USA
CoI: Nadia Zakamska, Johns Hopkins U.
CoI: Thaisa Storchi-Bergmann, UFRGS Brazil
CoI: Allan Schnorr-Muller, UFRGS Brazil
CoI: Jenny Greene, Princeton U.
CoI: Aleksandar Diamond-Stanic, U. of Wisconsin, Madison
CoI: Johan H Knapen, Instituto de Astrofisica de Canarias
CoI: Rongxin Luo, Shanghai Astronomical Observatory, China
CoI: Bililign Tsige Dullo, Instituto de Astrofisica de Canarias
Title: Probing AGN feedback models by zooming into active galaxies
Abstract: Supermassive black holes are strongly suspected to be key players in galaxy formation and evolution. Feedback from black hole accretion is implicated in establishing the black hole mass vs galaxy bulge correlations and in limiting the maximal stellar mass of galaxies, but direct observations of galaxy-wide feedback have been surprisingly difficult to obtain. We propose a GMOS integral field unit survey of 7 luminous active galactic nuclei (AGN) at z=0.03-0.15, covering optical diagnostic emission lines from HeII 4686 to [SII]6731, to detect and characterize AGN feedback. These observations combine Gemini data with the SDSS-MaNGA survey to probe physical scales between 250 pc and 8 kpc and to measure the power and extents of AGN-driven winds. With the 4-5 times better resolution at Gemini compared to MaNGA, we will be able to 'zoom into' the central kpc of the galaxy, investigating the origin and coupling of the wind to the outflowing gas. These data will allow us to probe the propagation of AGN-driven winds, discover young and/or stalled winds and determine whether AGN feedback affects star formation signatures in the host galaxy.
Program Type: Standard/Extragalactic
Run 1 (2016B): GEM-NQ/GMOSN -- 10.5hrs band 2 (GN-2016B-Q-62)
National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360