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Large scale kinematics and dynamical modelling of the Milky Way nuclear star cluster | Synapse

June 26, 2014Open Access

Large scale kinematics and dynamical modelling of the Milky Way nuclear star cluster

AFA. FeldmeierUniversity of Vienna NNNadine NeumayerMax Planck Institute for Astronomy ASAnil C. SethUniversity of Nebraska–Lincoln

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Resumen

Context. Within the central 10 pc of our Galaxy lies a dense cluster of stars. This nuclear star cluster forms a distinct component of the Galaxy, and similar nuclear star clusters are found in most nearby spiral and elliptical galaxies. Studying the structure and kinematics of nuclear star clusters reveals the history of mass accretion and growth of galaxy nuclei and central massive black holes.

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Feldmeier et al. (Thu,) studied this question.

synapsesocial.com/papers/6a1087e02badbc352a003513 https://doi.org/https://doi.org/10.1051/0004-6361/201423777

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