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 Radio Astronomy), 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(Max Planck Institute for Extraterrestrial Physics), Michael C. Cooper(University of California, Irvine), C. Feruglio(Institut de Radioastronomie Millimétrique), A. Saintonge(Max Planck Institute for Extraterrestrial Physics), Sirio Belli(Osservatorio astronomico di Bologna), D. Lutz(Max Planck Institute for Extraterrestrial Physics), E. Sturm(Max Planck Institute for Extraterrestrial Physics), Thomas Shimizu(Max Planck Institute for Extraterrestrial Physics), Stijn Wuyts(University of Bath), Jonathan Freundlich(Galaxies, Etoiles, Physique et Instrumentation), Alberto D. Bolatto(University of Maryland, College Park), Hannah Übler(University of Cambridge), F. Combes(Observatoire de Paris), Andreas Burkert(Max Planck Institute for Extraterrestrial Physics), 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(Max Planck Society)
The Astrophysical Journal
January 20, 2019
Cited by 80


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