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The rotational profiles of cluster galaxies

Bilton, Lawrence E; Hunt, Matthew; Pimbblet, Kevin A; Roediger, Elke

Authors

Lawrence E Bilton

Matthew Hunt

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Dr Elke Roediger E.Roediger@hull.ac.uk
Senior Lecturer/ Director of Studies for Physics



Abstract

© 2019 The Author(s) We compile two samples of cluster galaxies with complimentary hydrodynamic and N-body analysis using FLASH code to ascertain how their differing populations drive their rotational profiles and to better understand their dynamical histories.We select our main cluster sample from the X-ray Galaxy Clusters Database (BAX), which are populated with Sloan Digital Sky Survey (SDSS) galaxies. The BAX clusters are tested for the presence of substructures, acting as proxies for core mergers, culminating in sub-samples of eight merging and 25 non-merging galaxy clusters. An additional sample of 12 galaxy clusters with known dumbbell components is procured using galaxy data from the NASA/IPAC Extragalactic Database (NED) to compare against more extreme environments. BAX clusters of each sample are stacked on to a common RA-Dec. space to produce rotational profiles within the range of 0.0-2.5 r200. Merging stacks possess stronger core rotation at ≲0.5r200 primarily contributed by a red galaxy sub-population from relaxing core mergers; this is alongside high rotational velocities from blue galaxy sub-populations, until they mix and homogenize with the red sub-populations at ∼r200, indicative of an infalling blue galaxy sub-population with interactive mixing between both sub-populations at ≿ r200. FLASH code is utilized to simulate the merger phase between two originally independent clusters and test the evolution of their rotational profiles. Comparisons with the dumbbell clusters leads to the inference that the peculiar core rotations of some dumbbell clusters are the result of the linear motions of core galaxies relaxing on to the potential during post second infall.

Citation

Bilton, L. E., Hunt, M., Pimbblet, K. A., & Roediger, E. (2019). The rotational profiles of cluster galaxies. Monthly notices of the Royal Astronomical Society, 490(4), 5017-5032. https://doi.org/10.1093/mnras/stz2927

Journal Article Type Article
Acceptance Date Sep 10, 2019
Online Publication Date Oct 21, 2019
Publication Date Dec 1, 2019
Deposit Date Oct 28, 2019
Publicly Available Date Nov 26, 2019
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 490
Issue 4
Pages 5017-5032
DOI https://doi.org/10.1093/mnras/stz2927
Keywords Space and Planetary Science; Astronomy and Astrophysics; galaxies: clusters: general; galaxies: elliptical and lenticular; cD; galaxies: kinematics and dynamics
Public URL https://hull-repository.worktribe.com/output/2909470
Publisher URL https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stz2927/5601394

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Copyright Statement
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society







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