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...
Saved in:
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/8489/1/18_N._Hashim.pdf http://journalarticle.ukm.my/8489/ http://www.ukm.my/jsm/ |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The Nonlinear Least Square Fitting for Rotation Curve of Orion Dwarf Spiral
by: Roslan, Umar, et al.
Published: (2015) -
Dynamical structure of Orion dwarf galaxy / Muhammad Musoddiq Jaafar
by: Jaafar, Muhammad Musoddiq
Published: (2011) -
Preliminary analysis of investigation Radio Frequency Interference (RFI) profile analysis at Universiti Teknologi MARA
by: Roslan, Umar, et al.
Published: (2011) -
Probe team seeks 'Orion' and 'Delfin'
by: Anon
Published: (2017) -
Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia
by: Hamidi, Z.S., et al.
Published: (2012)