@techreport{848900eb239c40c4bddf62cf0d3a0ca6,
title = "The MAGPI Survey: Drivers of kinematic asymmetries in the ionised gas of $z\sim0.3$ star-forming galaxies",
abstract = "Galaxy gas kinematics are sensitive to the physical processes that contribute to a galaxy's evolution. It is expected that external processes will cause more significant kinematic disturbances in the outer regions, while internal processes will cause more disturbances for the inner regions. Using a subsample of 47 galaxies ($0.27",
keywords = "astro-ph.GA",
author = "Bagge, {R. S.} and C. Foster and A. Battisti and S. Bellstedt and M. Mun and K. Harborne and S. Barsanti and T. Mendel and S. Brough and Croom, {S. M.} and Lagos, {C. D. P.} and T. Mukherjee and Y. Peng and R-S Remus and G. Santucci and P. Sharda and S. Thater and Sande, {J. van de} and Zafar, {L. M. Valenzuela E. Wisnioski T.} and B. Ziegler",
note = "e.g., 20 pages, 19 figures",
year = "2023",
month = nov,
day = "17",
language = "English",
type = "WorkingPaper",
}