On the orbital periods for a particular case of spherical symmetry

A particular case of steady state and spherical symmetry - the so-called logarithmic potential introduced as the first approximation for dark coronae of galaxies - is studied. Both time and angle dependence of the distance to the centre for the orbit of a bound test particle with arbitrary initial c...

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Bibliographic Details
Main Authors: Ninković S., Jovanović B.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2008-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2008/1450-698X0876045N.pdf