Kinematic classifications of local interacting galaxies: Implications for the merger/disk classifications at high-z
The classification of galaxy mergers and isolated disks is key for understanding the relative importance of galaxy interactions and secular evolution during the assembly of galaxies. Galaxy kinematics as traced by emission lines have been used to suggest
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Hung_Kinematic_classifications_of_2015.pdf||3.68 MB||Adobe PDF|
|02_Hung_Kinematic_classifications_of_2015.pdf||3.68 MB||Adobe PDF|
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