On the Chermnykh-Like Problems: II. The Equilibrium Points

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dc.creatorYeh, Li-Chin
dc.creatorJiang, Ing-Guey
dc.date2006-10-26
dc.date.accessioned2026-07-07T10:24:00Z
dc.date.available2026-07-07T10:24:00Z
dc.descriptionMotivated by Papadakis (2005a, 2005b), we study a Chermnykh-like problem, in which an additional gravitational potential from the belt is included. In addition to the usual five equilibrium points (three collinear and two triangular points), there are some new equilibrium points for this system. We studied the conditions for the existence of these new equilibrium points both analytically and numerically.
dc.descriptionaccepted by Astrophysics and Space Science
dc.identifierhttps://arxiv.org/abs/astro-ph/0610767
dc.identifierhttp://arxiv.org/abs/astro-ph/0610767
dc.identifierAstrophys.SpaceSci.306:189-200,2006
dc.identifierdoi:10.1007/s10509-006-9170-4
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176039
dc.subjectAstrophysics
dc.titleOn the Chermnykh-Like Problems: II. The Equilibrium Points
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