On the evolution of simulated galaxies: the mass dependence in metallicity gradients
Abstract
Making use of a fiducial set of simulated disc galaxies spanning a wide range of mass, we examine the influence of stellar mass in the radial metallicity gradients and compare to observational trends from Ho et al. (2015).
- Publication:
-
Formation and Evolution of Galaxy Outskirts
- Pub Date:
- March 2017
- DOI:
- 10.1017/S1743921316008784
- Bibcode:
- 2017IAUS..321..302M