about
Cooling and clusters: when is heating needed?Energy distributions of symbiotic novaeTowards simulating star formation in the interstellar mediumAccretion shocks in clusters of galaxies and their SZ signature from cosmological simulationsConfusion of Diffuse Objects in the X-Ray SkyA comparison of cosmological hydrodynamic codesThe Impact of ICM Substructure on Ram Pressure StrippingOn the Origin of Intracluster EntropyModified Entropy Models for the Intracluster MediumRegulation of the X-ray luminosity of clusters of galaxies by cooling and supernova feedbackRegulation of star formation in giant galaxies by precipitation, feedback and conductionStatistical Properties of X‐Ray Clusters: Analytic and Numerical ComparisonsGas accretion is dominated by warm ionized gas in Milky Way mass galaxies at z ~ 0Ram pressure stripping of the Large Magellanic Cloud's disk as a probe of the Milky Way's circumgalactic mediumStar formation in ram pressure stripped galactic tailsHow to light it up: simulating ram-pressure stripped X-ray bright tailsERRATUM: “THE TAIL OF THE STRIPPED GAS THAT COOLED: H I, Hα, AND X-RAY OBSERVATIONAL SIGNATURES OF RAM PRESSURE STRIPPING” (2010, ApJ, 709, 1203)The tail of the stripped gas that cooled: H I, h{alpha}, and X-ray observational signatures of ram pressure strippingGas stripping in simulated galaxies with a multiphase interstellar mediumEnvironmentally Driven Evolution of Simulated Cluster GalaxiesConstraining intracluster gas models with AMiBA13Cosmological simulations of galaxy formation with cosmic raysImplications of Galaxy Buildup for Putative IMF Variations in Massive GalaxiesThe Impact of Galactic Winds on the Angular Momentum of Disk Galaxies in the Illustris SimulationA Global Model for Circumgalactic and Cluster-core PrecipitationCooling, AGN feedback, and star formation in simulated cool-core galaxy clustersPrecipitation-regulated star formation in galaxiesSupernova sweeping and black hole feedback in elliptical galaxiesNumerical Simulations of High‐Redshift Star Formation in Dwarf GalaxiesENZO: an adaptive mesh refinement code for astrophysicsA test suite for quantitative comparison of hydrodynamic codes in astrophysicsThe Effect of the Interstellar Model on Star Formation Properties in Galactic DisksThe Environmental Impact of Lyman Break GalaxiesSimulating Star Formation and Feedback in Galactic Disk ModelsAGN Heating in Simulated Cool-core ClustersModeling active galactic nucleus feedback in cool-core clusters: the balance between heating and coolingModeling active galactic nucleus feedback in cool-core clusters: the formation of cold clumpsSimulating the cooling flow of cool-core clustersA Quantification of the Butterfly Effect in Cosmological Simulations and Implications for Galaxy Scaling RelationsSimulating an isolated dwarf galaxy with multichannel feedback and chemical yields from individual stars
P50
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P50
description
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
Greg Bryan
@ast
Greg Bryan
@en
Greg Bryan
@es
Greg Bryan
@nl
type
label
Greg Bryan
@ast
Greg Bryan
@en
Greg Bryan
@es
Greg Bryan
@nl
prefLabel
Greg Bryan
@ast
Greg Bryan
@en
Greg Bryan
@es
Greg Bryan
@nl
P106
P21
P31
P496
0000-0003-2630-9228