On Cluster Rotation in the Galactic Tidal Field
Abstract: The dynamics of a rotating star cluster moving along a circular orbit in the axisymmetrical steady Galaxy is considered. The generalized tensor virial theorem allows to estimate its rotation speed. Conditions for direct and retrograde rotation in the galactic plane are found.
- Standort
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Deutsche Nationalbibliothek Frankfurt am Main
- Umfang
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Online-Ressource
- Sprache
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Englisch
- Erschienen in
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On Cluster Rotation in the Galactic Tidal Field ; volume:23 ; number:3-4 ; year:2014 ; pages:272-278 ; extent:7
Open astronomy ; 23, Heft 3-4 (2014), 272-278 (gesamt 7)
- Urheber
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Ossipkov, Leonid P.
- DOI
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10.1515/astro-2017-0191
- URN
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urn:nbn:de:101:1-2405271705103.555162029113
- Rechteinformation
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Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
- Letzte Aktualisierung
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14.08.2025, 10:58 MESZ
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Beteiligte
- Ossipkov, Leonid P.
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