Search Results - "Wetzel, Andrew R."
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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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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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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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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 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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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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Better Galactic Mass Models through Chemistry
Published in Galaxies (21-08-2017)“…With the upcoming release of the Gaia catalog and the many multiplexed spectroscopic surveys on the horizon, we are rapidly moving into a new data-driven era…”
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When the Jeans Do Not Fit: How Stellar Feedback Drives Stellar Kinematics and Complicates Dynamical Modeling in Low-mass Galaxies
Published in The Astrophysical journal (01-02-2017)“…In low-mass galaxies, stellar feedback can drive gas outflows that generate non-equilibrium fluctuations in the gravitational potential. Using cosmological…”
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Halo histories versus galaxy properties at z = 0 – III. The properties of star-forming galaxies
Published in Monthly notices of the Royal Astronomical Society (21-08-2018)“…ABSTRACT We measure how the properties of star-forming central galaxies correlate with large-scale environment, δ, measured on 10 h−1 Mpc scales. We use galaxy…”
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What determines satellite galaxy disruption?
Published in Monthly notices of the Royal Astronomical Society (01-04-2010)“…In hierarchical structure formation, dark matter haloes that merge with larger haloes can persist as subhaloes. These subhaloes are likely hosts of visible…”
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Simulating subhaloes at high redshift: merger rates, counts and types
Published in Monthly notices of the Royal Astronomical Society (21-05-2009)“…Galaxies are believed to be in one-to-one correspondence with simulated dark matter subhaloes. We use high-resolution N-body simulations of cosmological…”
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THE CONNECTION BETWEEN THE HOST HALO AND THE SATELLITE GALAXIES OF THE MILKY WAY
Published in The Astrophysical journal (20-10-2016)“…ABSTRACT Many properties of the Milky Way's (MW) dark matter halo, including its mass-assembly history, concentration, and subhalo population, remain poorly…”
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The clustering and host haloes of galaxy mergers at high redshift
Published in Monthly notices of the Royal Astronomical Society (21-04-2009)“…High-resolution simulations of cosmological structure formation indicate that dark matter substructure in dense environments, such as groups and clusters, may…”
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The Clustering of Massive Halos
Published in The Astrophysical journal (10-02-2007)“…The clustering properties of dark matter halos are a firm prediction of modern theories of structure formation. We use two large-volume, high-resolution…”
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Close Pairs as Proxies for Galaxy Cluster Mergers
Published in The Astrophysical journal (10-08-2008)“…Galaxy cluster merger statistics are an important component in understanding the formation of large-scale structure. Cluster mergers are also potential sources…”
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What determines satellite galaxy disruption?
Published in Monthly notices of the Royal Astronomical Society (01-04-2010)Get full text
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Halo histories versus Galaxy properties at z = 0 – I. The quenching of star formation
Published in Monthly notices of the Royal Astronomical Society (01-12-2017)Get full text
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The structure and dynamical evolution of the stellar disc of a simulated Milky Way-mass galaxy
Published in Monthly notices of the Royal Astronomical Society (11-05-2017)“…Abstract We study the structure, age and metallicity gradients, and dynamical evolution using a cosmological zoom-in simulation of a Milky Way-mass galaxy from…”
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