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

R. L. Davies, Stijn Wuyts(University of Bath), A. Renzini(Osservatorio Astronomico di Padova), R. Davies(Max Planck Institute for Extraterrestrial Physics), R. Genzel(Max Planck Institute for Extraterrestrial Physics), C. M. Carollo, Sandro Tacchella(University of Cambridge), C. Mancini(University of Padua), Rodrigo Herrera-Camus, Sirio Belli(Osservatorio astronomico di Bologna), 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(Max Planck Institute for Extraterrestrial Physics), 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(Max Planck Society)
The Astrophysical Journal
March 10, 2019
Cited by 109


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