Three-dimensional Keplerian orbit-superposition models of the nucleus of
M31

Three-dimensional Keplerian orbit-superposition models of the nucleus of M31

We present three-dimensional eccentric disc models of the nucleus of M31, modelling the disc as a linear combination of thick rings of massless stars orbiting in the potential of a central black hole. Our models are nonparametric generalisations of the parametric models of Peiris and Tremaine. The m...

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Dettagli Bibliografici
Autori principali:	Brown, C, Magorrian, S
Natura:	Journal article
Lingua:	English
Pubblicazione:	2013

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