Self-consistent modelling of the Milky Way’s nuclear stellar disc

Self-consistent modelling of the Milky Way’s nuclear stellar disc

The nuclear stellar disc (NSD) is a flattened high-density stellar structure that dominates the gravitational field of the Milky Way at Galactocentric radius $30\, {\rm pc}\lesssim R\lesssim 300\, {\rm pc}$. We construct axisymmetric self-consistent equilibrium dynamical models of the NSD in which t...

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Bibliografiska uppgifter
Huvudupphovsmän:	Sormani, MC, Sanders, JL, Fritz, TK, Smith, LC, Gerhard, O, Schödel, R, Magorrian, J, Neumayer, N, Nogueras-Lara, F, Feldmeier-Krause, A, Mastrobuono-Battisti, A, Schultheis, M, Shahzamanian, B, Vasiliev, E, Klessen, RS, Lucas, P, Minniti, D
Materialtyp:	Journal article
Språk:	English
Publicerad:	Oxford University Press 2022

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