Models of cuspy triaxial stellar systems - III. The effect of velocity anisotropy on chaoticity

In several previous investigations, we presented models of triaxial stellar systems, both cuspy and non-cuspy, that were highly stable and harboured large fractions of chaotic orbits. All our models had been obtained through cold collapses of initially spherical <i>N</i>-body systems, a...

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Detalles Bibliográficos
Autores principales:	Carpintero, Daniel Diego, Muzzio, Juan Carlos, Navone, Hugo Daniel
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2014
Materias:	Ciencias Astronómicas Chaos Galaxies: elliptical and lenticular, cD Galaxies: kinematics and dynamics Methods: numerical
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/85009
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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