On the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy
Abstract: An earlier derived quasi-isothermal Stäckel’s model of mass distribution in stellar systems and the corresponding formula for space density are applied to our Galaxy. The model rotation curve is fitted to HI kinematical data. The structural and scale parameters of the model are estimated and the corresponding density contours for our Galaxy are presented.
- 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 the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy ; volume:24 ; number:2 ; year:2015 ; pages:150-156 ; extent:7
Open astronomy ; 24, Heft 2 (2015), 150-156 (gesamt 7)
- Urheber
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Gromov, A. O.
Nikiforov, I. I.
Ossipkov, L. P.
- DOI
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10.1515/astro-2017-0214
- URN
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urn:nbn:de:101:1-2405271650228.876370517367
- Rechteinformation
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Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
- Letzte Aktualisierung
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14.08.2025, 10:49 MESZ
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Beteiligte
- Gromov, A. O.
- Nikiforov, I. I.
- Ossipkov, L. P.
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