Molecular and Ionized Gas Phases of an AGN-driven Outflow in a Typical Massive Galaxy at z ≈ 2

Rodrigo Herrera-Camus, A. Weiß(Max Planck Institute for Astrophysics), A. Renzini(Osservatorio Astronomico di Padova), S. García‐Burillo(Spanish National Observatory), R. Davies(Max Planck Institute for Extraterrestrial Physics), L. Colina(Consejo Superior de Investigaciones Científicas), R. Genzel(University of California, Berkeley), Michael C. Cooper(University of Arizona), C. Feruglio(Institut de Radioastronomie Millimétrique), A. Saintonge(Max Planck Institute for Extraterrestrial Physics), Sirio Belli(Max Planck Institute for Extraterrestrial Physics), D. Lutz(Max Planck Institute for Extraterrestrial Physics), E. Sturm(Max Planck Society), Thomas Shimizu(Max Planck Institute for Extraterrestrial Physics), Stijn Wuyts(Max Planck Institute for Extraterrestrial Physics), Jonathan Freundlich(Galaxies, Etoiles, Physique et Instrumentation), Alberto D. Bolatto(University of Maryland, College Park), Hannah Übler(University of Cambridge), F. Combes(Centre National de la Recherche Scientifique), Andreas Burkert(Ludwig-Maximilians-Universität München), P. Cox(Ausonius Institut de Recherche sur l'Antiquité et le Moyen age), L. J. Tacconi(Max Planck Institute for Extraterrestrial Physics), S. J. Lilly, N. M. Förster Schreiber(Max Planck Institute for Extraterrestrial Physics), Thorsten Naab(Ludwig-Maximilians-Universität München)
The Astrophysical Journal
January 20, 2019
Cited by 80


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