Models of cuspy triaxial stellar systems - I. Stability and chaoticity

We used the N-body code of Hernquist & Ostriker to build a dozen cuspy (γ ≃ 1) triaxial models of stellar systems through dissipationless collapses of initially spherical distributions of 10<SUP>6</SUP> particles. We chose four sets of initial conditions that resulted in models morph...

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Detalles Bibliográficos
Autores principales: Zorzi, Alejandra Francisca, Muzzio, Juan Carlos
Formato: Articulo
Lenguaje:Inglés
Publicado: 2012
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/83972
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