Determining the dark matter content of dwarfs and dwarfs spheroidal galaxies in the local group cluster using the CAS parameters

Determining the dark matter content of dwarfs and dwarfs spheroidal galaxies in the local group cluster using the CAS parameters

In this paper, we will discuss the CAS parameters (concentration, asymmetry and clumpiness) which are used to determine the non-parametric structures of dwarf samples to calculate the dark matter masses of dwarfs and dwarfs spheroidal galaxies in the Local Group Cluster. Dwarf galaxies are the most...

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Bibliographic Details
Published in:2011 IEEE International Conference on Space Science and Communication: "Towards Exploring the Equatorial Phenomena", IconSpace 2011 - Proceedings
Main Author: Ibrahim U.F.S.U.; Abidin Z.Z.; Hashim N.; Hassan M.S.R.; Hamidi Z.S.; Ibrahim Z.A.
Format: Conference paper
Language:English
Published: 2011
Online Access:https://www.scopus.com/inward/record.uri?eid=2-s2.0-80053228053&doi=10.1109%2fIConSpace.2011.6015879&partnerID=40&md5=1e4cfab4fccc56d90a2ac366b36ee7cc

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https://www.scopus.com/inward/record.uri?eid=2-s2.0-80053228053&doi=10.1109%2fIConSpace.2011.6015879&partnerID=40&md5=1e4cfab4fccc56d90a2ac366b36ee7cc

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