Non-linear stability in the perturbed photogravitational restricted three body problem

dc.contributor.author	Haque, M. N
dc.contributor.author	Ishwar, B
dc.date.accessioned	2007-09-14T07:35:15Z
dc.date.available	2007-09-14T07:35:15Z
dc.date.issued	1995
dc.identifier.citation	BASI, Vol. 23, No. 2, pp. 195-210	en
dc.identifier.uri	http://hdl.handle.net/2248/1788
dc.description.abstract	We have examined the non-linear stability of triangular equilibrium point in the perturbed photogravitaional restricted three body problem. We conclude that the equilibrium point is stable in the range of linear stability except for three mass ratio.	en
dc.format.extent	628154 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1995BASI...23..195H	en
dc.subject	stability	en
dc.subject	photogravitational	en
dc.subject	RTBP	en
dc.title	Non-linear stability in the perturbed photogravitational restricted three body problem	en
dc.type	Article	en