Stability of co-orbital motion in exoplanetary systems
type: Item
instance of: scholarly article
title: Stability of co-orbital motion in exoplanetary systems
zbMATH Open document ID: 1083.70015
author: Bálint Érdi
author: Zsolt Sándor
published in: Celestial Mechanics and Dynamical Astronomy
publication date: 2006-02-20T00:00:00Z
Mathematics Subject Classification ID: 70F15
Mathematics Subject Classification ID: 70F07
Mathematics Subject Classification ID: 70K20
zbMATH DE Number: 5007348
zbMATH Keywords: triangular Lagrangian points
zbMATH Keywords: relative Lyapunov indicators
zbMATH Keywords: elliptic restricted three-body problem
MaRDI profile type: Publication
full work available at URL: s10569-004-3114-5
OpenAlex ID: W2098475207
cites work: On the non-linear stability of motions around L5 in the elliptic restricted problem of the three bodies
cites work: The effect of eccentricity and inclination on the motion near the Lagrangian points \(L_4\) and \(L_5\)
cites work: The phase space structure around \(L_4\) in the restricted three-body problem
cites work: Symplectic mappings of co-orbital motion in the restricted problem of three bodies
cites work: Symplectic mapping for Trojan-type motion in the elliptic restricted three-body problem
cites work: The relative Lyapunov indicator: an efficient method of chaos detection
DOI: 10.1007/S10569-004-3114-5
description: scientific article; zbMATH DE number 5007348