The MAGPI Survey: Drivers of kinematic asymmetries in the ionised gas of z∼0.3 star-forming galaxies

2023/11/17 by R. S. Bagge, Caroline Foster, Bagge, R. S. +37
Chemistry · Physics and Astronomy · #Astrophysics and Star Formation Studies #Astrophysics of Galaxies (astro-ph.GA) #FOS: Physical sciences #Spectroscopy and Laser Applications #Stellar, planetary, and galactic studies

paper · pdf · doi:10.48550/arxiv.2311.10268

openalex publication_date 2023/11/17 · openalex created_date 2023/11/21 · openalex updated_date 2026/08/01

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

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