Relationship of the kinematic properties of cD galactic clusters to their radiative characteristics

A possible correlation between the dispersion in the velocities of regular galactic clusters and their total luminosity is discussed. Based on the generally accepted hypothesis that regular galactic clusters are equilibrated systems, we attempt to find a relationship similar to the Faber-Jackson rel...

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Published in:Astrophysics 2013-09, Vol.56 (3), p.359-369
Main Authors: Harutyunian, H. A., Harutyunyan, V. S.
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics
Astrophysics and Astroparticles
Astrophysics and Cosmology
Balancing
Cluster analysis
Clusters
Correlation
Dispersions
Galactic clusters
Galaxies
Kinematics
Luminosity
Observations and Techniques
Open clusters
Physics
Physics and Astronomy
Radiation
Space Exploration and Astronautics
Space Sciences (including Extraterrestrial Physics
Stars
Stars & galaxies
Studies
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Harutyunyan, V. S.
description A possible correlation between the dispersion in the velocities of regular galactic clusters and their total luminosity is discussed. Based on the generally accepted hypothesis that regular galactic clusters are equilibrated systems, we attempt to find a relationship similar to the Faber-Jackson relation between these quantities. The fact that no such relationship was found can be interpreted as a consequence of the incompleteness of the samples of galaxies that were used or, more likely, of the untenability of the assumption that these clusters are in equilibrium.
doi_str_mv 10.1007/s10511-013-9291-8
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1573-8191
language eng
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source Springer Nature
subjects Astronomy
Astrophysics
Astrophysics and Astroparticles
Astrophysics and Cosmology
Balancing
Cluster analysis
Clusters
Correlation
Dispersions
Galactic clusters
Galaxies
Kinematics
Luminosity
Observations and Techniques
Open clusters
Physics
Physics and Astronomy
Radiation
Space Exploration and Astronautics
Space Sciences (including Extraterrestrial Physics
Stars
Stars & galaxies
Studies
title Relationship of the kinematic properties of cD galactic clusters to their radiative characteristics
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