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...

Full description

Bibliographic Details
Published in:Sains Malaysiana
Main Author: 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: Penerbit Universiti Kebangsaan Malaysia 2015
Online Access:https://www.scopus.com/inward/record.uri?eid=2-s2.0-84983445534&doi=10.17576%2fjsm-2015-4403-18&partnerID=40&md5=1b3bd7e41314a6fbb325217ee7c2d4da

Similar Items