The nonlinear least square fitting for rotation curve of orion dwarf spiral

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The nonlinear least square fitting for rotation curve of orion dwarf spiral

The basis of the nonlinear least square fitting is to fit the nonlinear rotation curve model with the observed rotation curve of the Orion dwarf galaxy. It has been the most powerful tool to study the distribution of dark matter in galaxies where it is used to obtain the proper mass model of a galax...

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Bibliographic Details
Main Authors:	Hashim, N., Abidin, Z.Z., Ibrahim, U.F.S.U., Hassan, M.S.R., Hamidi, Z.S., Umar, R., Ibrahim, Z.A.
Format:	Article
Language:	English
Published:	Universiti Kebangsaan Malaysia 2015
Online Access:	http://journalarticle.ukm.my/8489/ http://journalarticle.ukm.my/8489/1/18_N._Hashim.pdf

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