Simulation of the loss-cone instability in spherical systems: II. Dominating Keplerian potential

ABSTRACT. According to our previous theoretical findings, physical processes in centres of galaxies, star clusters, and the Oort comet cloud can be significant

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Bibliographische Detailangaben
Hauptverfasser: Polyachenko, Evgeny V. (VerfasserIn) , Just, Andreas (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2020 January 17
In: Monthly notices of the Royal Astronomical Society
Year: 2020, Jahrgang: 492, Heft: 4, Pages: 4819-4824
ISSN:1365-2966
DOI:10.1093/mnras/staa141
Online-Zugang:Verlag, Volltext: https://doi.org/10.1093/mnras/staa141
Verlag: https://academic.oup.com/mnras/article/492/4/4819/5708945
Volltext
Verfasserangaben:E.V. Polyachenko, P. Berczik, A. Just and I.G. Shukhman

MARC

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