Possible Relations between Brightest Central Galaxies and Their Host Galaxies Clusters and Groups

The r-band of the Sloan Digital Sky Survey (SDSS) for 17,924 brightest cluster galaxies (BCGs) in clusters and groups within 0.02 ⩽ z ⩽ 0.20 are used to study possible environmental relations affecting the nature of these galaxies. We find a correlation between BCGs physical properties (the effectiv...

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Main Authors: Samir R. M., Shaker A. A.
Format: Article
Language:English
Published: Sciendo 2021-01-01
Series:Applied Mathematics and Nonlinear Sciences
Subjects:
Online Access:https://doi.org/10.2478/amns.2021.1.00002
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author Samir R. M.
Shaker A. A.
author_facet Samir R. M.
Shaker A. A.
author_sort Samir R. M.
collection DOAJ
description The r-band of the Sloan Digital Sky Survey (SDSS) for 17,924 brightest cluster galaxies (BCGs) in clusters and groups within 0.02 ⩽ z ⩽ 0.20 are used to study possible environmental relations affecting the nature of these galaxies. We find a correlation between BCGs physical properties (the effective radius (Re), absolute magnitude and central velocity dispersion (σ0)) and their host groups and clusters velocity dispersion (σcl). This type of relations suggests that the most massive groups or clusters host larger central galaxies. On the other hand, the σ0/σcl ratio as a function of σcl is consistent with [10].
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spelling doaj.art-486e942ff02649a7a0cd3269e47c321d2022-12-22T03:13:50ZengSciendoApplied Mathematics and Nonlinear Sciences2444-86562021-01-016239540010.2478/amns.2021.1.00002Possible Relations between Brightest Central Galaxies and Their Host Galaxies Clusters and GroupsSamir R. M.0Shaker A. A.1Galactic and Extragalactic Laboratory, Astronomy Department, National Research Institute of Astronomy and Geophysics (NRIAG), Helwan – 11421 - Cairo, Egypt.Galactic and Extragalactic Laboratory, Astronomy Department, National Research Institute of Astronomy and Geophysics (NRIAG), Helwan – 11421 - Cairo, Egypt.The r-band of the Sloan Digital Sky Survey (SDSS) for 17,924 brightest cluster galaxies (BCGs) in clusters and groups within 0.02 ⩽ z ⩽ 0.20 are used to study possible environmental relations affecting the nature of these galaxies. We find a correlation between BCGs physical properties (the effective radius (Re), absolute magnitude and central velocity dispersion (σ0)) and their host groups and clusters velocity dispersion (σcl). This type of relations suggests that the most massive groups or clusters host larger central galaxies. On the other hand, the σ0/σcl ratio as a function of σcl is consistent with [10].https://doi.org/10.2478/amns.2021.1.00002brightest central galaxiesbcgsgalaxy clustersgalaxy groups85-0885a0585a15
spellingShingle Samir R. M.
Shaker A. A.
Possible Relations between Brightest Central Galaxies and Their Host Galaxies Clusters and Groups
Applied Mathematics and Nonlinear Sciences
brightest central galaxies
bcgs
galaxy clusters
galaxy groups
85-08
85a05
85a15
title Possible Relations between Brightest Central Galaxies and Their Host Galaxies Clusters and Groups
title_full Possible Relations between Brightest Central Galaxies and Their Host Galaxies Clusters and Groups
title_fullStr Possible Relations between Brightest Central Galaxies and Their Host Galaxies Clusters and Groups
title_full_unstemmed Possible Relations between Brightest Central Galaxies and Their Host Galaxies Clusters and Groups
title_short Possible Relations between Brightest Central Galaxies and Their Host Galaxies Clusters and Groups
title_sort possible relations between brightest central galaxies and their host galaxies clusters and groups
topic brightest central galaxies
bcgs
galaxy clusters
galaxy groups
85-08
85a05
85a15
url https://doi.org/10.2478/amns.2021.1.00002
work_keys_str_mv AT samirrm possiblerelationsbetweenbrightestcentralgalaxiesandtheirhostgalaxiesclustersandgroups
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