Influence of baryonic physics on the merger timescale of galaxies in N-body/hydrodynamical simulations

Astronomy and Astrophysics

Volumn 510, Issue 1, 2010, Pages

  Jiang, C Y ^a,b   Jing, Y P ^a   Lin, W P ^a  

^a CHINESE ACADEMY OF SCIENCES   (China)

^b UNIVERSITY OF CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

Galaxies: clusters: general; Galaxies: kinematics and dynamics; Methods: numerical

Indexed keywords

EXTREME CASE; FITTING FORMULA; GALAXIES: CLUSTERS: GENERAL; GALAXIES: KINEMATICS AND DYNAMICS; HIGH RESOLUTION; LIMITING CASE; METHODS: NUMERICAL; NUMERICAL IMPLEMENTATION; STELLAR MASS; TIME-SCALES;

COMPUTER SIMULATION; DYNAMICS; KINEMATICS; MERGERS AND ACQUISITIONS; MERGING; NUMERICAL METHODS; STARS;

GALAXIES;

EID: 79952854472     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913257     Document Type: Article

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