The Dynamical Evolution of a Star Cluster

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DC Field	Value	Language
dc.contributor.author	Sunder, G. S	-
dc.contributor.author	Kochhar, R. K	-
dc.date.accessioned	2008-09-22T11:49:36Z	-
dc.date.available	2008-09-22T11:49:36Z	-
dc.date.issued	1987	-
dc.identifier.citation	IAU Symposium, No. 127, pp. 525 - 526	en
dc.identifier.issn	0074-1809	-
dc.identifier.uri	http://hdl.handle.net/2248/3763	-
dc.description.abstract	Using the second order tensor virial equations and the equation for the rate of change of the kinetic energy tensor, the authors follow the dynamical evolution of a star cluster with anisotropic velocity distribution. They show that the cluster executes finite amplitude oscillations both in size and eccentricity. However, unlike in the isotropic case, the amplitude now depends on the initial eccentricity.	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1987IAUS..127..525S	en
dc.subject	Star cluster	en
dc.title	The Dynamical Evolution of a Star Cluster	en
dc.type	Article	en
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