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(University of Bath), Thorsten Naab(Max Planck Society), David J. Wilman(Max Planck Institute for Extraterrestrial Physics), R. Davies(Max Planck Institute for Extraterrestrial Physics), R. Genzel(Max Planck Institute for Extraterrestrial Physics), Ken-ichi Tadaki(National Astronomical Observatory of Japan), Matteo Fossati(Brera Astronomical Observatory), P. Lang(Max Planck Institute for Astronomy), A. Beifiori(Max Planck Institute for Extraterrestrial Physics), Rodrigo Herrera-Camus, Sirio Belli(Osservatorio astronomico di Bologna), Maximilian Fabricius(Max Planck Institute for Extraterrestrial Physics), J. Trevor Mendel(Australian National University), D. Lutz(Max Planck Institute for Extraterrestrial Physics), R. Bender(Max Planck Institute for Extraterrestrial Physics), 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(Max Planck Institute for Extraterrestrial Physics), 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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