Models of cuspy triaxial stellar systems – IV. Rotating systems

We built two self-consistent models of triaxial, cuspy, rotating stellar systems adding rotation to non-rotating models presented in previous papers of this series. The final angular velocity of the material is not constant and varies with the distance to the centre and with the height over the equa...

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Detalles Bibliográficos
Autores principales:	Carpintero, Daniel Diego, Muzzio, Juan Carlos
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2016
Materias:	Ciencias Astronómicas methods: numerical galaxies: elliptical and lenticular, cD galaxies: kinematics and dynamics
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/123896
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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