about
The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3.Galaxy formation with BECDM - I. Turbulence and relaxation of idealized haloes.Galaxy motions cause trouble for cosmology.The Importance of Preventive Feedback: Inference from Observations of the Stellar Masses and Metallicities of Milky Way Dwarf GalaxiesThe connection between the host halo and the satellite galaxies of the Milky WaySegue 2: the least massive galaxyDynamical friction and galaxy merging time-scalesThe merger rates and mass assembly histories of dark matter haloes in the two Millennium simulationsThe mass–concentration–redshift relation of cold dark matter haloesGalactic accretion and the outer structure of galaxies in the CDM modelThe mass profile and accretion history of cold dark matter haloesThe Proper Motion of Pyxis: The First Use of Adaptive Optics in Tandem withHSTon a Faint Halo ObjectDDO 216-A1: A Central Globular Cluster in a Low-luminosity Transition-type GalaxyThe mass dependence of satellite quenching in Milky Way-like haloesM31 satellite masses compared to ΛCDM subhaloesA dichotomy in satellite quenching around L* galaxiesSmall-scale structure in the Sloan Digital Sky Survey and {Lambda}CDM: isolated ~L_*_ galaxies with bright satellitesFurther constraining galaxy evolution models through the size function of SDSS early-type galaxiesThe density and pseudo-phase-space density profiles of cold dark matter haloesFrom dwarf spheroidals to cD galaxies: simulating the galaxy population in a ΛCDM cosmologyThe statistics of the subhalo abundance of dark matter haloesThere's no place like home? Statistics of Milky Way-mass dark matter haloesResolving cosmic structure formation with the Millennium-II SimulationSimulating galaxies in the reionization era with FIRE-2: galaxy scaling relations, stellar mass functions, and luminosity functionsDiscrete Effects in Stellar Feedback: Individual Supernovae, Hypernovae, and IMF Sampling in Dwarf GalaxiesFIRE-2 simulations: physics versus numerics in galaxy formationSimulating galaxies in the reionization era with FIRE-2: morphologies and sizesHow to model supernovae in simulations of star and galaxy formationSIDM on FIRE: hydrodynamical self-interacting dark matter simulations of low-mass dwarf galaxies.The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulationsNot so lumpy after all: modelling the depletion of dark matter subhaloes by Milky Way-like galaxiesForged in fire: cusps, cores and baryons in low-mass dwarf galaxiesSweating the small stuff: simulating dwarf galaxies, ultra-faint dwarf galaxies, and their own tiny satellitesDwarf galaxy mass estimators versus cosmological simulationsThe origin of ultra diffuse galaxies: stellar feedback and quenchingGas kinematics in FIRE simulated galaxies compared to spatially unresolved H i observationsGas kinematics, morphology and angular momentum in the FIRE simulationsWhat drives the evolution of gas kinematics in star-forming galaxies?Warm FIRE: Simulating Galaxy Formation with Resonant Sterile Neutrino Dark MatterWhere are the most ancient stars in the Milky Way?
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description
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
M Boylan-Kolchin
@ast
M Boylan-Kolchin
@en
M Boylan-Kolchin
@es
M Boylan-Kolchin
@nl
type
label
M Boylan-Kolchin
@ast
M Boylan-Kolchin
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M Boylan-Kolchin
@es
M Boylan-Kolchin
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prefLabel
M Boylan-Kolchin
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M Boylan-Kolchin
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M Boylan-Kolchin
@es
M Boylan-Kolchin
@nl
P106
P31
P496
0000-0002-9604-343X