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Titlebook: Symmetries and Dynamics of Star Clusters; Jaroslav Haas Book 2014 Springer International Publishing Switzerland 2014 Dynamics of Star Clus

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樓主: mountebank
11#
發(fā)表于 2025-3-23 13:40:35 | 只看該作者
Dynamical Coupling of Near-Keplerian Orbits,del of active galactic nuclei. Hence, in Chap. 3 of the thesis, we analyse the gravitational influence of such a structure upon the orbital evolution of an initially thin stellar disc around a supermassive black hole which is embedded in an extended spherical star cluster.
12#
發(fā)表于 2025-3-23 14:09:06 | 只看該作者
Book 2014igates the orbital evolution of an initially thin stellar disc around a supermassive black hole, considering various perturbative sources of gravity. His findings, obtained by both direct numerical N-body modelling and using standard perturbation methods, offer a viable theoretical explanation for t
13#
發(fā)表于 2025-3-23 20:07:29 | 只看該作者
2190-5053 planation for the observed configuration of young stars in t.In this PhD thesis, which was nominated for publication in this series by the Astronomical Institute at Charles University, Prague, the author investigates the orbital evolution of an initially thin stellar disc around a supermassive black
14#
發(fā)表于 2025-3-24 01:03:31 | 只看該作者
Prerequisites,ee-body problem, leading then to description of relaxational processes in N-body systems. We particularly focus on the case of central mass dominated systems, such as isolated thin stellar discs around supermassive black holes.
15#
發(fā)表于 2025-3-24 03:55:54 | 只看該作者
Thin Disc Embedded in Extended Spherically Symmetric Cluster,onable to expect these stellar discs to be embedded in extended spherically symmetric star clusters. Hence, in Chap. 2 of the thesis, we investigate the orbital evolution of an initially thin stellar disc under the gravitational influence of such a spherical star cluster.
16#
發(fā)表于 2025-3-24 09:57:49 | 只看該作者
Dynamical Coupling of Near-Keplerian Orbits,del of active galactic nuclei. Hence, in Chap. 3 of the thesis, we analyse the gravitational influence of such a structure upon the orbital evolution of an initially thin stellar disc around a supermassive black hole which is embedded in an extended spherical star cluster.
17#
發(fā)表于 2025-3-24 13:38:46 | 只看該作者
18#
發(fā)表于 2025-3-24 17:24:32 | 只看該作者
https://doi.org/10.1007/978-3-319-03650-2Dynamics of Star Clusters; Feeding of supermassive black holes; Galactic Center; Galactic Centre; Galact
19#
發(fā)表于 2025-3-24 20:11:07 | 只看該作者
20#
發(fā)表于 2025-3-25 01:50:06 | 只看該作者
Conclusions,In the last chapter of the thesis, we conclude our research.
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