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Disk dominated galaxies retain their shapes below $z = 1.0$
Author(s) -
Kai Hoffmann,
C. Laigle,
Nora Elisa Chisari,
Pau Tallada,
Yohan Dubois,
Julien Devriendt
Publication year - 2020
Publication title -
cornell university
Language(s) - Uncategorized
DOI - 10.5167/uzh-193016
Subject(s) - physics , astrophysics , bulge , galaxy , redshift , radius , galaxy formation and evolution , lenticular galaxy , peculiar galaxy , mass distribution , astronomy , computer security , computer science

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