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2008MNRAS.391.1373B - Mon. Not. R. Astron. Soc., 391, 1373-1383 (2008/December-2)
On the axisymmetric thin disc model of flattened galaxies.
BRATEK L., JALOCHA J. and KUTSCHERA M.
Abstract (from CDS):
It has also been found that the baryonic matter distribution in the spiral galaxy NGC 5475, obtained in the axisymmetric thin disc approximation, accounts for the rotation curve of the galaxy. To obtain these results, the iteration method developed recently by the authors has been applied.
Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS
Journal keyword(s): gravitation - methods: analytical - methods: numerical - galaxies: kinematics and dynamics - galaxies: luminosity function, mass function - galaxies: spiral
Simbad objects: 5
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