Old Web
English
Sign In
Acemap
>
Paper
>
The Evolution and Origin of Ionized Gas Velocity Dispersion from z ∼ 2.6 to z ∼ 0.6 with KMOS3D
The Evolution and Origin of Ionized Gas Velocity Dispersion from z ∼ 2.6 to z ∼ 0.6 with KMOS3D
2019
Hannah Übler
R. Genzel
Emily Wisnioski
N. M. Förster Schreiber
T. Shimizu
Sedona H. Price
L. J. Tacconi
Sirio Belli
D.J. Wilman
M. Fossati
J. T. Mendel
R. L. Davies
A. Beifiori
Ralf Bender
Gabe Brammer
Andreas Burkert
J. Chan
R. I. Davies
M. Fabricius
A. Galametz
R. Herrera-Camus
Philipp A. Lang
D. Lutz
Ivelina Momcheva
Thorsten Naab
Erica J. Nelson
R. P. Saglia
Ken-Ichi Tadaki
P. G. van Dokkum
Stijn Wuyts
Keywords:
Plasma
Astrophysics
Physics
Velocity dispersion
Correction
Cite
Save
Machine Reading By IdeaReader
0
References
0
Citations
NaN
KQI
[]