Kiloparsec Scale Properties of Star Formation Driven Outflows at z ∼ 2.3 in the SINS/zC-SINF AO Survey*

R. L. Davies, Stijn Wuyts(Max Planck Institute for Extraterrestrial Physics), A. Renzini(Osservatorio Astronomico di Padova), R. Davies(Max Planck Institute for Extraterrestrial Physics), R. Genzel(University of California, Berkeley), C. M. Carollo, Sandro Tacchella(ETH Zurich), C. Mancini(University of Padua), Rodrigo Herrera-Camus, Sirio Belli(Max Planck Institute for Extraterrestrial Physics), D. Lutz(Max Planck Institute for Extraterrestrial Physics), Thomas Shimizu(Max Planck Institute for Extraterrestrial Physics), Hannah Übler(University of Cambridge), A. Sternberg(Tel Aviv University), Erica J. Nelson(Planetary Science Institute), Andreas Burkert(Ludwig-Maximilians-Universität München), Sedona H. Price(Max Planck Institute for Extraterrestrial Physics), L. J. Tacconi(Max Planck Institute for Extraterrestrial Physics), Emily Wisnioski(Australian National University), S. J. Lilly, N. M. Förster Schreiber(Max Planck Institute for Extraterrestrial Physics), Thorsten Naab(Ludwig-Maximilians-Universität München)
The Astrophysical Journal
March 10, 2019
Cited by 109


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