activity
20112026
most citedThe Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time

568 citations · 8.7k across the 176 of their papers we have counts for

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Showing 2019Show all

20 papers · 1 filter

astro-ph.GA2019★ 37 cited

Structural and photometric properties of barred galaxies from the Auriga cosmological simulations

Guillermo Blázquez-Calero, Estrella Florido, Isabel Pérez +6

In this work we analyse the structural and photometric properties of 21 barred simulated galaxies from the Auriga Project. These consist of Milky Way-mass magneto-hydrodynamical si…

astro-ph.GA2019★ 79 cited

Magnetising the circumgalactic medium of disk galaxies

Ruediger Pakmor, Freeke van de Voort, Rebekka Bieri +7

The circumgalactic medium (CGM) is one of the frontiers of galaxy formation and intimately connected to the galaxy via accretion of gas on to the galaxy and gaseous outflows from t…

astro-ph.GA2019★ 157 cited

Chemodynamics of barred galaxies in cosmological simulations: On the Milky Way's quiescent merger history and in-situ bulge

F. Fragkoudi, R. J. J. Grand, R. Pakmor +9

We explore the chemodynamical properties of a sample of barred galaxies in the Auriga magneto-hydrodynamical cosmological zoom-in simulations, which form boxy/peanut (b/p) bulges,…

astro-ph.GA2019★ 343 cited

The Milky Way total mass profile as inferred from Gaia DR2

Marius Cautun, Alejandro Benitez-Llambay, Alis J. Deason +7

We determine the Milky Way (MW) mass profile inferred from fitting physically motivated models to the Gaia DR2 Galactic rotation curve and other data. Using various hydrodynamical…

astro-ph.GA2019★ 107 cited

The effects of cosmic rays on the formation of Milky Way-mass galaxies in a cosmological context

Tobias Buck, Christoph Pfrommer, Rüdiger Pakmor +2

We investigate the impact of cosmic rays (CR) and different modes of CR transport on the properties of Milky Way-mass galaxies in cosmological magneto-hydrodynamical simulations in…

astro-ph.GA2019★ 111 cited

Gas accretion and galactic fountain flows in the Auriga cosmological simulations: angular momentum and metal re-distribution

Robert J. J. Grand, Freeke van de Voort, Jolanta Zjupa +7

Using a set of 15 high-resolution magnetohydrodynamic cosmological simulations of Milky Way formation, we investigate the origin of the baryonic material found in stars at redshift…

astro-ph.GA2019★ 55 cited

Dark matter halo shapes in the Auriga simulations

Jesus Prada, Jaime E. Forero-Romero, Robert J. J. Grand +2

We present shape measurements of Milky Way-sized dark matter halos at redshift in a suite of 30 zoom simulations from the Auriga project. We compare the results in full magne…

astro-ph.GA2019★ 31 cited

The dark matter component of the Gaia radially anisotropic substructure

Nassim Bozorgnia, Azadeh Fattahi, Carlos S. Frenk +5

We study the properties of the dark matter component of the radially anisotropic stellar population recently identified in the Gaia data, using magneto-hydrodynamical simulations o…

astro-ph.GA2019★ 298 cited

The Biggest Splash

Vasily Belokurov, Jason L. Sanders, Azadeh Fattahi +4

Using a large sample of bright nearby stars with accurate Gaia Data Release 2 astrometry and auxiliary spectroscopy we map out the properties of the principle Galactic components s…

astro-ph.GA2019★ 19 cited

The globular cluster system of the Auriga simulations

Timo L. R. Halbesma, Robert J. J. Grand, Facundo A. Gómez +5

We investigate whether the galaxy and star formation model used for the Auriga simulations can produce a realistic globular cluster (GC) population. We compare statistics of GC can…

astro-ph.GA2019★ 21 cited

The diversity of the circumgalactic medium around z = 0 Milky Way-mass galaxies from the Auriga simulations

Maan H. Hani, Sara L. Ellison, Martin Sparre +4

Galaxies are surrounded by massive gas reservoirs (i.e. the circumgalactic medium; CGM) which play a key role in their evolution. The properties of the CGM, which are dependent on…

astro-ph.GA2019★ 61 cited

The prevalence of pseudo-bulges in the Auriga simulations

Ignacio D. Gargiulo, Antonela Monachesi, Facundo A. Gómez +7

We study the galactic bulges in the Auriga simulations, a suite of thirty cosmological magneto-hydrodynamical zoom-in simulations of late-type galaxies in Milky Way-sized dark matt…

astro-ph.GA2019★ 83 cited

Neutron star mergers and rare core-collapse supernovae as sources of r-process enrichment in simulated galaxies

Freeke van de Voort, Rüdiger Pakmor, Robert J. J. Grand +3

We use cosmological, magnetohydrodynamical simulations of Milky Way-mass galaxies from the Auriga project to study their enrichment with rapid neutron capture (r-process) elements.…

astro-ph.GA2019★ 55 cited

The effects of dynamical substructure on Milky Way mass estimates from the high velocity tail of the local stellar halo

Robert J. J. Grand, Alis J. Deason, Simon D. M. White +4

We investigate the impact of dynamical streams and substructure on estimates of the local escape speed and total mass of Milky Way-mass galaxies from modelling the high velocity ta…

astro-ph.GA2019★ 34 cited

A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations

Dandan Xu, Ling Zhu, Robert Grand +16

Motivated by the recently discovered kinematic "Hubble sequence" shown by the stellar orbit-circularity distribution of 260 CALIFA galaxies, we make use of a comparable galaxy samp…

astro-ph.GA2019★ 32 cited

WARPFIELD Population Synthesis: The physics of (extra-)Galactic star formation and feedback driven cloud structure and emission from sub-to-kpc scales

E. W. Pellegrini, S. Reissl, D. Rahner +5

We present a novel method to model galactic scale star formation and the resulting emission from star clusters and the multi-phase interstellar medium. We combine global parameters…

astro-ph.GA2019★ 22 cited

Simulating cosmological substructure in the solar neighbourhood

Christine M. Simpson, Ignacio Gargiulo, Facundo A. Gómez +8

We explore the predictive power of cosmological, hydrodynamical simulations for stellar phase space substructure and velocity correlations with the Auriga simulations and Aurigaia…

astro-ph.GA2019★ 83 cited

Ultra-diffuse galaxies in the Auriga simulations

Shihong Liao, Liang Gao, Carlos S. Frenk +7

We investigate the formation of ultra-diffuse galaxies (UDGs) using the Auriga high-resolution cosmological magneto-hydrodynamical simulations of Milky Way-sized galaxies. We ident…

astro-ph.GA2019★ 32 cited

Satellites of Satellites: The Case for Carina and Fornax

Stephen A. Pardy, Elena D'Onghia, Julio Navarro +6

We use the Auriga cosmological simulations of Milky Way (MW)-mass galaxies and their surroundings to study the satellite populations of dwarf galaxies in CDM. As expected from p…

astro-ph.GA2019★ 118 cited

The local high velocity tail and the Galactic escape speed

Alis J. Deason, Azadeh Fattahi, Vasily Belokurov +4

We model the fastest moving (v_tot > 300 km/s) local (D < 3 kpc) halo stars using cosmological simulations and 6-dimensional Gaia data. Our approach is to use our knowledge of the…