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...
Guardado en:
| Autores principales: | Zorzi, Alejandra Francisca, Muzzio, Juan Carlos |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2012
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/83972 |
| Aporte de: |
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