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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Format: | Article |
Language: | English |
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2021-01-01
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Series: | Applied Mathematics and Nonlinear Sciences |
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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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id | doaj.art-486e942ff02649a7a0cd3269e47c321d |
institution | Directory Open Access Journal |
issn | 2444-8656 |
language | English |
last_indexed | 2024-04-12T22:37:09Z |
publishDate | 2021-01-01 |
publisher | Sciendo |
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series | Applied Mathematics and Nonlinear Sciences |
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 AT shakeraa possiblerelationsbetweenbrightestcentralgalaxiesandtheirhostgalaxiesclustersandgroups |