The Evolution and Origin of Ionized Gas Velocity Dispersion from z ∼ 2.6 to z ∼ 0.6 with KMOS<sup>3D</sup> <sup>∗</sup>

Hannah Übler(University of Cambridge), Stijn Wuyts(Max Planck Institute for Extraterrestrial Physics), Thorsten Naab(Ludwig-Maximilians-Universität München), David J. Wilman(Max Planck Institute for Extraterrestrial Physics), R. Davies(Max Planck Institute for Extraterrestrial Physics), R. Genzel(University of California, Berkeley), Ken-ichi Tadaki(National Astronomical Observatory of Japan), Matteo Fossati(Durham University), P. Lang(Max Planck Institute for Astronomy), A. Beifiori(Max Planck Institute for Extraterrestrial Physics), Rodrigo Herrera-Camus, Sirio Belli(Max Planck Institute for Extraterrestrial Physics), Maximilian Fabricius(Max Planck Institute for Extraterrestrial Physics), J. Trevor Mendel(Australian National University), D. Lutz(Max Planck Institute for Extraterrestrial Physics), R. Bender(Institut d'Astrophysique de Paris), Ivelina Momcheva(Yale University), Thomas Shimizu(Max Planck Institute for Extraterrestrial Physics), J. Chan(University of California, Riverside), Pieter van Dokkum(Yale University), R. L. Davies, Erica J. Nelson(Planetary Science Institute), Andreas Burkert(Ludwig-Maximilians-Universität München), Gabriel Brammer(University of Copenhagen), Sedona H. Price(Max Planck Institute for Extraterrestrial Physics), L. J. Tacconi(Max Planck Institute for Extraterrestrial Physics), Emily Wisnioski(Australian National University), R. P. Saglia(Max Planck Institute for Extraterrestrial Physics), N. M. Förster Schreiber(Max Planck Institute for Extraterrestrial Physics), A. Galametz(University of Geneva)
The Astrophysical Journal
July 20, 2019
Cited by 169


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