293 citations · 1.9k across the 50 of their papers we have counts for
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NIHAO XIII: Clumpy discs or clumpy light in high redshift galaxies?
Tobias Buck, Andrea V. Macciò, Aura Obreja +3
Many massive star forming disc galaxies in the redshift range 3 to 0.5 are observed to have a clumpy morphology showing giant clumps of size 1 kpc and masses of about $10^7M_…
Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift
David Goz, Pierluigi Monaco, Gian Luigi Granato +5
We present predictions of Spectral Energy Distributions (SEDs), from the UV to the FIR, of simulated galaxies at . These were obtained by post-processing the results of an N-b…
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…
NIHAO XI: Formation of Ultra-Diffuse Galaxies by outflows
Arianna Di Cintio, Chris B. Brook, Aaron A. Dutton +3
We address the origin of Ultra-Diffuse Galaxies (UDGs), which have stellar masses typical of dwarf galaxies but effective radii of Milky Way-sized objects. Their formation mechanis…
NIHAO X: Reconciling the local galaxy velocity function with Cold Dark Matter via mock HI observations
Andrea V. Macciò, Silviu M. Udrescu, Aaron A. Dutton +4
We used 87 high resolution hydrodynamical cosmological simulations from the NIHAO suite to investigate the relation between the maximum circular velocity (Vmax) of a dark matter ha…
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…