1 code implementation • 5 Sep 2019 • Timo L. R. Halbesma, Robert J. J. Grand, Facundo A. Gómez, Federico Marinacci, Rüdiger Pakmor, Wilma H. Trick, Philipp Busch, Simon D. M. White
We find that the Auriga simulations do produce sufficient stellar mass for GC candidates at radii and metallicities that are typical for the MW GC system (GCS).
Astrophysics of Galaxies
1 code implementation • 14 Jan 2019 • J. Ted Mackereth, Jo Bovy, Henry W. Leung, Ricardo P. Schiavon, Wilma H. Trick, William J. Chaplin, Katia Cunha, Diane K. Feuillet, Steven R. Majewski, Marie Martig, Andrea Miglio, David Nidever, Marc H. Pinsonneault, Victor Silva Aguirre, Jennifer Sobeck, Jamie Tayar, Gail Zasowski
Outer disc populations also have flatter radial AVRs than those in the inner disc, likely due to the waning effect of spiral arms.
Astrophysics of Galaxies
