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A numerical simulation of galaxy subcluster mergersWe present preliminary results of a 3-D numerical simulation of two merging subclusters of galaxies. By self-consistently modelling the intracluster gas and dark matter dynamics, we hope to gain insight as to how the dynamics of both relate to such observables as the cluster x-ray emission, radio source morphology, and velocity dispersions.
Document ID
19930017644
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Roettiger, Kurt (New Mexico State Univ. Las Cruces, NM, United States)
Burns, Jack O. (New Mexico State Univ. Las Cruces, NM, United States)
Loken, Chris (New Mexico State Univ. Las Cruces, NM, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1993
Publication Information
Publication: NASA. Ames Research Center, The Evolution of Galaxies and Their Environment
Subject Category
Astrophysics
Accession Number
93N26833
Funding Number(s)
CONTRACT_GRANT: NSF AST-90-12353
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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