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On the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Jun 2015Embargo end date: 01 Jan 2015 English Publisher:Walter de Gruyter GmbHJournal:Open Astronomy, volume 24, pages 150-156 (eissn: 2543-6376, Copyright policy )
Authors: Gromov A. O.; Nikiforov I. I.; Ossipkov L. P.;

doi: 10.1515/astro-2017-0214 , 10.48550/arxiv.1508.05298

arXiv: 1508.05298

On the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy

Abstract

AbstractAn 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.

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Keywords

Astronomy, Astrophysics of Galaxies (astro-ph.GA), galaxy: kinematics and dynamics, FOS: Physical sciences, QB1-991, Astrophysics - Astrophysics of Galaxies, methods: analytical

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
1
Average
Average
Average
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gold
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