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Jalocha, J., Bratek, L. and Kutschera, M. (2008) Is Dark Matter Present in NGC 4736? An Iterative Spectral Method for Finding Mass Distribution in Spiral Galaxies. The Astrophysical Journal, 679, 373-378.
https://doi.org/10.1086/533511

has been cited by the following article:

• TITLE: On the Characteristic Acceleration of MOND

  AUTHORS: Barbaro Quintero-Leyva

  KEYWORDS: Dark Matter, Galaxies: Kinematics and Dynamics, Cosmology

  JOURNAL NAME: Open Access Library Journal, Vol.4 No.4, April 26, 2017

  ABSTRACT: The impact of the geometry on the gravitational force field and the impact of the mass beyond the test particle location were assessed in the rotation curve calculation of a hypothetical thin disk galaxy using Newtonian and Mondian dynamics. An effective equation for the characteristic acceleration of MOND was obtained based on the Mestel’s finite disk by normalizing the line mass density to the total mass of the galaxy and equating it to the theoretical value.