Sensitivity of the orbital content of a model stellar system to the potential approximation used to describe it

DOI10.1007/S10569-006-9039-4zbMath1116.85001OpenAlexW2046814305WikidataQ107365301 ScholiaQ107365301MaRDI QIDQ868501

Felipe C. Wachlin, Daniel D. Carpintero

Publication date: 5 March 2007

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: http://sedici.unlp.edu.ar/handle/10915/130461

zbMATH Keywords

Numerical methodsStellar orbitsTriaxial stellar systems

Mathematics Subject Classification ID

Computational methods for problems pertaining to mechanics of particles and systems (70-08) Celestial mechanics (70F15) Galactic and stellar dynamics (85A05)

Related Items (2)

Orbital structure of self-consistent cuspy triaxial stellar systems ⋮ Orbital structure of self-consistent triaxial stellar systems

Cites Work

• Spatial structure of regular and chaotic orbits in a self-consistent triaxial stellar system
• Unnamed Item

This page was built for publication: Sensitivity of the orbital content of a model stellar system to the potential approximation used to describe it