The MAGPI Survey

Autor(en)
R. S. Bagge, C. Foster, A. Battisti, S. Bellstedt, M. Mun, K. Harborne, S. Barsanti, T. Mendel, S. Brough, S. M. Croom, C. D. P. Lagos, T. Mukherjee, Y. Peng, R-S Remus, G. Santucci, P. Sharda, S. Thater, J. van de Sande, L. M. Valenzuela E. Wisnioski T. Zafar, B. Ziegler
Abstrakt

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

Organisation(en)
Institut für Astrophysik
Publikationsdatum
11-2023
ÖFOS 2012
103004 Astrophysik
Schlagwörter
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/848900eb-239c-40c4-bddf-62cf0d3a0ca6