Search Results - "Gómez, Facundo A"
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Hunting for the Dark Matter Wake Induced by the Large Magellanic Cloud
Published in The Astrophysical journal (10-10-2019)“…Satellite galaxies are predicted to generate gravitational density wakes as they orbit within the dark matter (DM) halos of their hosts, causing their orbits…”
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The Orbital Histories of Magellanic Satellites Using Gaia DR2 Proper Motions
Published in The Astrophysical journal (01-04-2020)“…With the release of Gaia DR2, it is now possible to measure the proper motions (PMs) of the lowest-mass, ultrafaint satellite galaxies in the Milky Way's (MW)…”
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Quenching and ram pressure stripping of simulated Milky Way satellite galaxies
Published in Monthly notices of the Royal Astronomical Society (21-07-2018)“…Abstract We present predictions for the quenching of star formation in satellite galaxies of the Local Group from a suite of 30 cosmological zoom simulations…”
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The influence of Sagittarius and the Large Magellanic Cloud on the stellar disc of the Milky Way Galaxy
Published in Monthly notices of the Royal Astronomical Society (21-11-2018)Get full text
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The mass of the Milky Way from satellite dynamics
Published in Monthly notices of the Royal Astronomical Society (21-04-2019)“…Abstract We present and apply a method to infer the mass of the Milky Way (MW) by comparing the dynamics of MW satellites to those of model satellites in the…”
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Footprints of the Sagittarius dwarf galaxy in the Gaia data set
Published in Monthly notices of the Royal Astronomical Society (21-05-2019)“…ABSTRACT We analyse an N-body simulation of the interaction of the Milky Way (MW) with a Sagittarius-like dSph (Sgr), looking for signatures which may be…”
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Vertical disc heating in Milky Way-sized galaxies in a cosmological context
Published in Monthly notices of the Royal Astronomical Society (11-06-2016)“…Vertically extended, high velocity dispersion stellar distributions appear to be a ubiquitous feature of disc galaxies, and both internal and external…”
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The effect of magnetic fields on properties of the circumgalactic medium
Published in Monthly notices of the Royal Astronomical Society (01-03-2021)“…ABSTRACT We study the effect of magnetic fields on a simulated galaxy and its surrounding gaseous halo, or circumgalactic medium (CGM), within cosmological…”
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The mass of the Milky Way out to 100 kpc using halo stars
Published in Monthly notices of the Royal Astronomical Society (01-03-2021)“…ABSTRACT We use a distribution function analysis to estimate the mass of the Milky Way (MW) out to 100 kpc using a large sample of halo stars. These stars are…”
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Gas accretion and galactic fountain flows in the Auriga cosmological simulations: angular momentum and metal redistribution
Published in Monthly notices of the Royal Astronomical Society (01-12-2019)“…ABSTRACT Using a set of 15 high-resolution magnetohydrodynamic cosmological simulations of Milky Way formation, we investigate the origin of the baryonic…”
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Neutron star mergers and rare core-collapse supernovae as sources of r-process enrichment in simulated galaxies
Published in Monthly notices of the Royal Astronomical Society (01-06-2020)“…ABSTRACT We use cosmological, magnetohydrodynamical simulations of Milky Way-mass galaxies from the Auriga project to study their enrichment with rapid neutron…”
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Warps and waves in the stellar discs of the Auriga cosmological simulations
Published in Monthly notices of the Royal Astronomical Society (01-03-2017)“…Recent studies have revealed an oscillating asymmetry in the vertical structure of the Milky Way's disc. Here, we analyse 16 high-resolution, fully…”
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THE CATERPILLAR PROJECT: A LARGE SUITE OF MILKY WAY SIZED HALOS
Published in The Astrophysical journal (10-02-2016)“…ABSTRACT We present the largest number of Milky Way sized dark matter halos simulated at very high mass (∼104 /particle) and temporal resolution (5…”
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The Auriga stellar haloes: connecting stellar population properties with accretion and merging history
Published in Monthly notices of the Royal Astronomical Society (11-05-2019)“…Abstract We examine the stellar haloes of the Auriga simulations, a suite of 30 cosmological magnetohydrodynamical high-resolution simulations of Milky…”
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A tale of two populations: surviving and destroyed dwarf galaxies and the build-up of the Milky Way’s stellar halo
Published in Monthly notices of the Royal Astronomical Society (01-10-2020)“…ABSTRACT We use magnetohydrodynamical simulations of Milky Way-mass haloes from the Auriga project to investigate the properties of surviving and destroyed…”
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The milky way total mass profile as inferred from Gaia DR2
Published in Monthly notices of the Royal Astronomical Society (21-05-2020)“…ABSTRACT We determine the Milky Way (MW) mass profile inferred from fitting physically motivated models to the Gaia DR2 Galactic rotation curve and other data…”
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Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation
Published in Monthly notices of the Royal Astronomical Society (01-11-2021)“…ABSTRACT We investigate the formation of the satellite galaxy population of a Milky Way-mass halo in a very highly resolved magnetohydrodynamic cosmological…”
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The multiplicity and anisotropy of galactic satellite accretion
Published in Monthly notices of the Royal Astronomical Society (11-05-2018)“…Abstract We study the incidence of group and filamentary dwarf galaxy accretion into Milky Way (MW) mass haloes using two types of hydrodynamical simulations:…”
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Descendants of the first stars: the distinct chemical signature of second-generation stars
Published in Monthly notices of the Royal Astronomical Society (01-08-2018)“…ABSTRACT Extremely metal-poor (EMP) stars in the Milky Way (MW) allow us to infer the properties of their progenitors by comparing their chemical composition…”
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The origin of galactic metal-rich stellar halo components with highly eccentric orbits
Published in Monthly notices of the Royal Astronomical Society (21-04-2019)“…Abstract Using the astrometry from the ESA’s Gaia mission, previous works have shown that the Milky Way stellar halo is dominated by metal-rich stars on highly…”
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