about
Cold, clumpy accretion onto an active supermassive black hole.Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxiesUltraviolet morphology and unobscured UV star formation rates of CLASH brightest cluster galaxiesA Global Model for Circumgalactic and Cluster-core PrecipitationCooling, AGN feedback, and star formation in simulated cool-core galaxy clustersENZO: an adaptive mesh refinement code for astrophysicsThe Effects of Ram Pressure on the Cold Clouds in the Centers of Galaxy ClustersAGN 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 clustersDetermining the Dust Extinction of Gamma-ray Burst Host Galaxies: A Direct Method Based on Optical and X-ray Photometry
P50
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P50
description
researcher
@en
հետազոտող
@hy
name
Yuan Li
@ast
Yuan Li
@en
Yuan Li
@es
Yuan Li
@nl
type
label
Yuan Li
@ast
Yuan Li
@en
Yuan Li
@es
Yuan Li
@nl
prefLabel
Yuan Li
@ast
Yuan Li
@en
Yuan Li
@es
Yuan Li
@nl
P106
P31
P496
0000-0001-5262-6150