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Galaxy clusters are the most massive gravitationally bound structures in the universe with a mass range of 1012 M ≤ M ≤ 1015 M. Galaxy clusters play an important role in observational cosmology due to their their bound and relaxed structures because their evolution is directly re...

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محفوظ في:
التفاصيل البيبلوغرافية
المؤلف الرئيسي: ACHMAD RESDIANSYAH (NIM : 10309026); Pembimbing : Dr. Yayan Sugianto, SANDY
التنسيق: Final Project
اللغة:Indonesia
الوصول للمادة أونلاين:https://digilib.itb.ac.id/gdl/view/20512
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المؤسسة: Institut Teknologi Bandung
اللغة: Indonesia
id id-itb.:20512
spelling id-itb.:205122017-09-27T11:42:17Z#TITLE_ALTERNATIVE# ACHMAD RESDIANSYAH (NIM : 10309026); Pembimbing : Dr. Yayan Sugianto, SANDY Indonesia Final Project INSTITUT TEKNOLOGI BANDUNG https://digilib.itb.ac.id/gdl/view/20512 Galaxy clusters are the most massive gravitationally bound structures in the universe with a mass range of 1012 M &#8804; M &#8804; 1015 M. Galaxy clusters play an important role in observational cosmology due to their their bound and relaxed structures because their evolution is directly related to the growth of cosmic structures, especially large-scale structures. Clusters are ideal <br /> <br /> <br /> laboratories for studying interactions between galaxies and the effect on galaxy population because of their high densities. <br /> <br /> <br /> In this Thesis, we will discuss the Abell 0957 cluster which is one of the first clusters studied by George O. Abell in 1958 in his catalogue. After much data compiling using a statistical approach by Bukhari & Cram by calculating the mean and deviations of the radial velocity v and projected distance from the cluster center r, we have determined the physical properties of <br /> <br /> <br /> the custer among others redshift = 0,0565, comoving distance = 239 Mpc, 61 member galaxies, and a cluster radius of 0,95 Mpc. During the data compilation, a group of galaxies in the neighborhood of Abell 0957 have been sighted and the Bukhari-Cram method will be used to <br /> <br /> <br /> determine the detected groups. text
institution Institut Teknologi Bandung
building Institut Teknologi Bandung Library
continent Asia
country Indonesia
Indonesia
content_provider Institut Teknologi Bandung
collection Digital ITB
language Indonesia
description Galaxy clusters are the most massive gravitationally bound structures in the universe with a mass range of 1012 M &#8804; M &#8804; 1015 M. Galaxy clusters play an important role in observational cosmology due to their their bound and relaxed structures because their evolution is directly related to the growth of cosmic structures, especially large-scale structures. Clusters are ideal <br /> <br /> <br /> laboratories for studying interactions between galaxies and the effect on galaxy population because of their high densities. <br /> <br /> <br /> In this Thesis, we will discuss the Abell 0957 cluster which is one of the first clusters studied by George O. Abell in 1958 in his catalogue. After much data compiling using a statistical approach by Bukhari & Cram by calculating the mean and deviations of the radial velocity v and projected distance from the cluster center r, we have determined the physical properties of <br /> <br /> <br /> the custer among others redshift = 0,0565, comoving distance = 239 Mpc, 61 member galaxies, and a cluster radius of 0,95 Mpc. During the data compilation, a group of galaxies in the neighborhood of Abell 0957 have been sighted and the Bukhari-Cram method will be used to <br /> <br /> <br /> determine the detected groups.
format Final Project
author ACHMAD RESDIANSYAH (NIM : 10309026); Pembimbing : Dr. Yayan Sugianto, SANDY
spellingShingle ACHMAD RESDIANSYAH (NIM : 10309026); Pembimbing : Dr. Yayan Sugianto, SANDY
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author_facet ACHMAD RESDIANSYAH (NIM : 10309026); Pembimbing : Dr. Yayan Sugianto, SANDY
author_sort ACHMAD RESDIANSYAH (NIM : 10309026); Pembimbing : Dr. Yayan Sugianto, SANDY
title #TITLE_ALTERNATIVE#
title_short #TITLE_ALTERNATIVE#
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url https://digilib.itb.ac.id/gdl/view/20512
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