Benjamin W Keller

TL;DR: The Gasoline2 as mentioned in this paper is the most recent version of the Gasoline code for parallel hydrodynamics and gravity with identical hydroynamics to the Changa code.

TL;DR: In this article, the authors used high resolution Hydro+N-Body cosmological simulations to compare the assembly and evolution of a small field dwarf (stellar mass ∼ 10 6 7 M, total mass 10 10 M) indominated CDM and 2keV WDM cosmologies and found that star for-mation (SF) in the WDM model is reduced and delayed by 1-2 Gyr relative to the CDM model, independently of the details of SF and feedback.

TL;DR: In this article, the authors examine the importance of stochasticity due to discreteness noise, variations in merger timings and how self-regulation moderates the effects of this stochasticallyity.

TL;DR: In this paper, a suite of hydrodynamical simulations of isolated galaxies containing a spheroid was performed to investigate the impact of these morphological components on star formation, and the most bulge-dominated galaxies showed the strongest deviation from the main sequence.