The MAGPI survey: Drivers of kinematic asymmetries in the ionised gas of z 0.3 star-forming galaxies
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA（2023）
摘要
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更多
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关键词
galaxies: evolution,galaxies: formation,galaxies: interactions,galaxies: ISM,galaxies: kinematics and dynamics,galaxies: star formation
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