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20032018
most citedStar Formation and Feedback in Smoothed Particle Hydrodynamic Simulations--I. Isolated Galaxies

749 citations · 2.1k across the 12 of their papers we have counts for

collaborators

22 papers

astro-ph.GA2018

Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy

Aura Obreja, Andrea V. Macciò, Benjamin Moster +4

We present the first results of applying Gaussian Mixture Models in the stellar kinematic space of normalized angular momentum and binding energy on NIHAO high resolution galaxies…

astro-ph.GA2018

NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes

Aura Obreja, Aaron A. Dutton, Andrea V. Macciò +6

We use 25 simulated galaxies from the NIHAO project to define and characterize a variety of kinematic stellar structures: thin and thick discs, large scale single discs, classical…

astro-ph.GA2017★ 7 cited

Haloes at the ragged edge: The importance of the splashback radius

O. N. Snaith, J. Bailin, A. Knebe +3

We have explored the outskirts of dark matter haloes out to 2.5 times the virial radius using a large sample of halos drawn from Illustris, along with a set of zoom simulations (MU…

astro-ph.GA2017★ 4 cited

Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model

Thales A. Gutcke, Andrea V. Macciò, Aaron A. Dutton +1

The decrease in star formation (SF) and the morphological change necessary to produce the elliptical galaxy population are commonly ascribed to a sudden quenching event, whic…

astro-ph.GA2016

NIHAO XII: galactic uniformity in a ΛCDM universe

Aaron A. Dutton, Aura Obreja, Liang Wang +7

We use a sample of 83 high-resolution cosmological zoom-in simulations and a semi-analytic model (SAM) to study the stochasticity of galaxy formation in haloes ranging from dwarf t…

astro-ph.GA2016

NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes

Aaron A. Dutton, Andrea V. Macciò, Avishai Dekel +7

We use ~100 cosmological galaxy formation zoom-in simulations using the smoothed particle hydrodynamics code {\sc gasoline} to study the effect of baryonic processes on the mass pr…