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
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2020 January 17
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| 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 |
| Verfasserangaben: | E.V. Polyachenko, P. Berczik, A. Just and I.G. Shukhman |
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