© 2018 The Author(s). We present an analysis of the kinematics of a sample of 14 galaxy clusters via velocity dispersion profiles (VDPs), compiled using cluster parameters defined within the X-Ray Galaxy Clusters Database (BAX) cross-matched with data from the Sloan Digital Sky Survey (SDSS). We determine the presence of substructure in the clusters from the sample as a proxy for recent core mergers, resulting in 4 merging and 10 non-merging clusters to allow for comparison between their respective dynamical states. We create VDPs for our samples and divide them by mass, colour, and morphology to assess how their kinematics respond to the environment. To improve the signal-to-noise ratio our galaxy clusters are normalized and co-added to a ...
Aims. The relationship between baryonic and dark components in galaxies varies with the environment ...
Context. The processes responsible for galaxy evolution in different environments as a function of g...
We study the fraction of tidal interactions and mergers with well identified observability timescale...
© 2018 The Author(s). We present an analysis of the kinematics of a sample of 14 galaxy clusters via...
© 2019 The Author(s) We compile two samples of cluster galaxies with complimentary hydrodynamic and ...
© 2020 The Author(s) We produce a kinematic analysis of AGN-hosting cluster galaxies from a sample o...
Galaxy clusters represent one of the largest-scale structures in the Universe, with their environmen...
Galaxy clusters represent one of the largest-scale structures in the Universe, with their en- vironm...
I present a study of the merger rate of galaxies in various cluster environments. Mergers are thoug...
Context.Large surveys such as the Sloan Digital Sky Survey have made large amounts of spectroscopic ...
ABSTRACT We measure the velocity dispersions of clusters of galaxies selected by the red-se...
An extensive redshift survey has been conducted on a sample of 15 nearby (0.01 < z < 0.05) clusters ...
Velocity dispersion profiles and rotation curves have been determined for a sample of 13 brightest d...
Context. We study the distribution of galaxies in nearby clusters to shed light on the evolutionary ...
Aims. The relationship between baryonic and dark components in galaxies varies with the environment ...
Context. The processes responsible for galaxy evolution in different environments as a function of g...
We study the fraction of tidal interactions and mergers with well identified observability timescale...
© 2018 The Author(s). We present an analysis of the kinematics of a sample of 14 galaxy clusters via...
© 2019 The Author(s) We compile two samples of cluster galaxies with complimentary hydrodynamic and ...
© 2020 The Author(s) We produce a kinematic analysis of AGN-hosting cluster galaxies from a sample o...
Galaxy clusters represent one of the largest-scale structures in the Universe, with their environmen...
Galaxy clusters represent one of the largest-scale structures in the Universe, with their en- vironm...
I present a study of the merger rate of galaxies in various cluster environments. Mergers are thoug...
Context.Large surveys such as the Sloan Digital Sky Survey have made large amounts of spectroscopic ...
ABSTRACT We measure the velocity dispersions of clusters of galaxies selected by the red-se...
An extensive redshift survey has been conducted on a sample of 15 nearby (0.01 < z < 0.05) clusters ...
Velocity dispersion profiles and rotation curves have been determined for a sample of 13 brightest d...
Context. We study the distribution of galaxies in nearby clusters to shed light on the evolutionary ...
Aims. The relationship between baryonic and dark components in galaxies varies with the environment ...
Context. The processes responsible for galaxy evolution in different environments as a function of g...
We study the fraction of tidal interactions and mergers with well identified observability timescale...