dc.contributor.author |
Namboodiri, P. M. S |
|
dc.date.accessioned |
2008-08-13T05:08:55Z |
|
dc.date.available |
2008-08-13T05:08:55Z |
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dc.date.issued |
2000-02 |
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dc.identifier.citation |
Celestial Mechanics and Dynamical Astronomy, Vol. 76, No. 1, pp. 69 - 77 |
en |
dc.identifier.issn |
0923-2958 |
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dc.identifier.uri |
http://hdl.handle.net/2248/3101 |
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dc.description |
Restricted Access |
en |
dc.description.abstract |
Oscillations in galaxies have been investigated by numerical simulations. The various models used have density distributions corresponding to that of polytrope of index n in the range 0 ≤ n ≤ 4 and their evolution has been followed for more than 70 crossing times. The kinetic energy shows regular and smooth oscillations for models with n = 0, 1 and 2 whereas in other models it shows noisy oscillation. The oscillation in kinetic energy is observed to have a period of 3 crossing time irrespective of the density and size of the galaxy. The amplitude of oscillation is seen to decrease as the central density of the galaxy increases. |
en |
dc.format.extent |
102660 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Springer |
en |
dc.relation.uri |
http://www.springerlink.com/content/n5780g2kh4244280/ |
en |
dc.subject |
Stellar Dynamics |
en |
dc.subject |
Galaxies |
en |
dc.subject |
Oscillations |
en |
dc.subject |
Numerical Simulations |
en |
dc.title |
Oscillations In Galaxies |
en |
dc.type |
Article |
en |