about
Gas loss in simulated galaxies as they fall into clustersThe relationship between dietary factors and serum lipids in southern Chinese population samples.Multilocus sequence typing (MLST) analysis of 104 Clostridium difficile strains isolated from China.Long noncoding RNA HOXD-AS1 regulates proliferation of cervical cancer cells by activating Ras/ERK signaling pathway.Observations of the missing baryons in the warm–hot intergalactic mediumA hydrodynamic approach to cosmology: The mixed dark matter cosmological scenarioThe Lyα Forest Power Spectrum from the Sloan Digital Sky SurveyA Constraint on the Gravitational Lensing Magnification and Age of the Redshiftz = 6.28 Quasar SDSS 1030+0524The Most Ancient Spiral Galaxy: A 2.6-Gyr-old Disk with a Tranquil Velocity FieldA comparison of cosmological hydrodynamic codesLarge-scale clustering of Lyman α emission intensity from SDSS/BOSSCan standard cosmological models explain the observed Abell cluster bulk flow?Massive Galaxies and Extremely Red Objects atz= 1–3 in Cosmological Hydrodynamic Simulations: Near‐Infrared PropertiesMassive Galaxies in Cosmological Simulations: Ultraviolet‐selected Sample at Redshiftz = 2Is There a Missing Galaxy Problem at High Redshift?Comparisons of cosmological magnetohydrodynamic galaxy cluster simulations to radio observationsCosmoMHD: A Cosmological Magnetohydrodynamics CodeCosmological Mestel Disks and the Rossby Vortex Instability: The Origin of Supermassive Black HolesConstraining Ω with Cluster EvolutionDetermining the Amplitude of Mass Fluctuations in the UniverseProbing the Dependence of the Intergalactic Medium on Large-scale Environment Using the Low-redshift Lyα ForestDo not forget the forest for the trees: the stellar-mass halo-mass relation in different environmentsOn the reversal of star formation rate-density relation at z = 1: insights from simulationsEffects on galaxy evolution: pair interactions versus environmentTesting the Large-scale Environments of Cool-core and Non-cool-core Clusters with Clustering BiasProposed SMEX to spectrally analyze the diffuse x-ray background: The Baryonic Extragalactic Structure Tracer (BEST)ENZO: an adaptive mesh refinement code for astrophysicsSupernova feedback and the hot gas filling fraction of the interstellar mediumAlleviating the scaling problem of cosmological hydrodynamic simulations with HECAGalaxy size problem at z = 3: simulated galaxies are too smallBaryons in the Warm‐Hot Intergalactic MediumThe Metal Enrichment and Temperature of the Intergalactic MediumA piecewise parabolic method for cosmological hydrodynamicsX-ray clusters from a high-resolution hydrodynamic PPM simulation of the cold dark matter universeThe Local Group as a test of cosmological models21cmfast: a fast, seminumerical simulation of the high-redshift 21-cm signalComparison of reionization models: radiative transfer simulations and approximate, seminumeric modelsImplications of the Lyα Emission Line from a Candidate z = 10 GalaxyProbing the Reionization History Using the Spectra of High‐Redshift SourcesCosmic Reionization and the 21 cm Signal: Comparison between an Analytical Model and a Simulation
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P50
description
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
Renyue Cen
@ast
Renyue Cen
@en
Renyue Cen
@es
Renyue Cen
@nl
type
label
Renyue Cen
@ast
Renyue Cen
@en
Renyue Cen
@es
Renyue Cen
@nl
prefLabel
Renyue Cen
@ast
Renyue Cen
@en
Renyue Cen
@es
Renyue Cen
@nl
P214
P106
P214
P31
P496
0000-0001-8531-9536
P7859
lccn-nr90028776