Search Results - "Wetzel, Andrew"
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On the orbits of infalling satellite haloes
Published in Monthly notices of the Royal Astronomical Society (21-03-2011)“…The orbital properties of infalling satellite haloes set the initial conditions which control the subsequent evolution of subhaloes and the galaxies that they…”
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Galaxy evolution in groups and clusters: star formation rates, red sequence fractions and the persistent bimodality
Published in Monthly notices of the Royal Astronomical Society (01-07-2012)“…Using galaxy group/cluster catalogues created from the Sloan Digital Sky Survey Data Release 7, we examine in detail the specific star formation rate (SSFR)…”
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SATELLITE DWARF GALAXIES IN A HIERARCHICAL UNIVERSE: INFALL HISTORIES, GROUP PREPROCESSING, AND REIONIZATION
Published in The Astrophysical journal (01-07-2015)“…ABSTRACT In the Local Group (LG), almost all satellite dwarf galaxies that are within the virial radius of the Milky Way (MW) and Andromeda (M31) exhibit…”
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THE PHYSICAL NATURE OF THE COSMIC ACCRETION OF BARYONS AND DARK MATTER INTO HALOS AND THEIR GALAXIES
Published in The Astrophysical journal (20-07-2015)“…ABSTRACT The cosmic accretion of both dark matter and baryons into halos is typically measured using some evolving virial relation, but recent work suggests…”
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Galaxy evolution in groups and clusters: satellite star formation histories and quenching time-scales in a hierarchical Universe
Published in Monthly notices of the Royal Astronomical Society (11-06-2013)“…Satellite galaxies in groups and clusters are more likely to have low star formation rates (SFRs) and lie on the 'red sequence' than central ('field')…”
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Gaia Reveals a Metal-rich, in situ Component of the Local Stellar Halo
Published in The Astrophysical journal (20-08-2017)“…We use the first Gaia data release, combined with the RAVE and APOGEE spectroscopic surveys, to investigate the origin of halo stars within kpc from the Sun…”
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Baryonic solutions and challenges for cosmological models of dwarf galaxies
Published in Nature astronomy (01-08-2022)“…Galaxies and their dark-matter haloes have posed several challenges to the dark energy plus cold dark matter ( Λ CDM) cosmological model. These discrepancies…”
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Black holes on FIRE: stellar feedback limits early feeding of galactic nuclei
Published in Monthly notices of the Royal Astronomical Society. Letters (21-11-2017)“…Abstract We introduce massive black holes (BHs) in the Feedback In Realistic Environments (FIRE) project and perform high-resolution cosmological hydrodynamic…”
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AGN All the Way Down? AGN-like Line Ratios Are Common in the Lowest-mass Isolated Quiescent Galaxies
Published in The Astrophysical journal (20-10-2019)“…We investigate the lowest-mass quiescent galaxies known to exist in isolated environments ( ; 1.5 Mpc from a more massive galaxy). This population may…”
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The Local Group on FIRE: dwarf galaxy populations across a suite of hydrodynamic simulations
Published in Monthly notices of the Royal Astronomical Society (01-07-2019)“…Abstract We present a new set of high-resolution hydrodynamic cosmological zoom-in simulations that apply the Feedback In Realistic Environments physics to…”
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BREATHING FIRE: HOW STELLAR FEEDBACK DRIVES RADIAL MIGRATION, RAPID SIZE FLUCTUATIONS, AND POPULATION GRADIENTS IN LOW-MASS GALAXIES
Published in The Astrophysical journal (01-04-2016)“…ABSTRACT We examine the effects of stellar feedback and bursty star formation on low-mass galaxies (Mstar = 2 × 106 − 5 × 1010 M ) using the Feedback in…”
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FIRE-2 simulations: physics versus numerics in galaxy formation
Published in Monthly notices of the Royal Astronomical Society (11-10-2018)Get full text
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fire in the field: simulating the threshold of galaxy formation
Published in Monthly notices of the Royal Astronomical Society (01-11-2017)“…Abstract We present a suite of 15 cosmological zoom-in simulations of isolated dark matter haloes, all with masses of M halo ≈ 1010 M⊙ at z = 0, in order to…”
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What does Clustering Tell us About the Buildup of the Red Sequence?
Published in The Astrophysical journal (10-08-2010)“…We analyze the clustering of red and blue galaxies from four samples spanning a redshift range of 0.4 < z < 2.0 to test the various scenarios by which galaxies…”
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Star Formation Quenching Timescale of Central Galaxies in a Hierarchical Universe
Published in The Astrophysical journal (20-05-2017)“…Central galaxies make up the majority of the galaxy population, including the majority of the quiescent population at . Thus, the mechanism(s) responsible for…”
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Gas kinematics, morphology and angular momentum in the FIRE simulations
Published in Monthly notices of the Royal Astronomical Society (01-01-2018)“…Abstract We study the z = 0 gas kinematics, morphology and angular momentum content of isolated galaxies in a suite of cosmological zoom-in simulations from…”
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The origins of the circumgalactic medium in the FIRE simulations
Published in Monthly notices of the Royal Astronomical Society (01-09-2019)“…ABSTRACT We use a particle tracking analysis to study the origins of the circumgalactic medium (CGM), separating it into (1) accretion from the intergalactic…”
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Halo histories versus galaxy properties at z = 0 II: large-scale galactic conformity
Published in Monthly notices of the Royal Astronomical Society (11-06-2018)“…Abstract Using group catalogues from the Sloan Digital Sky Survey (SDSS) Data Release 7, we measure galactic conformity in the local universe. We measure the…”
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Galaxy evolution near groups and clusters: ejected satellites and the spatial extent of environmental quenching
Published in Monthly notices of the Royal Astronomical Society (11-04-2014)“…Galaxies that are several virial radii beyond groups/clusters show preferentially quiescent star formation rates (SFR). Using a galaxy group/cluster catalogue…”
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The formation times and building blocks of Milky Way-mass galaxies in the FIRE simulations
Published in Monthly notices of the Royal Astronomical Society (01-09-2020)“…ABSTRACT Surveys of the Milky Way (MW) and M31 enable detailed studies of stellar populations across ages and metallicities, with the goal of reconstructing…”
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