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Stäackel-type Dynamic Model of the Galaxy Based on Maser Kinematic Data

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Mar 2016Embargo end date: 01 Jan 2016 English Publisher:Walter de Gruyter GmbHJournal:Open Astronomy, volume 25, pages 53-59 (eissn: 2543-6376, Copyright policy )
Authors: A. O. Gromov; L. P. Ossipkov; I. I. Nikiforov;

doi: 10.1515/astro-2017-0110 , 10.48550/arxiv.1609.04283

arXiv: http://arxiv.org/abs/1609.04283

Stäackel-type Dynamic Model of the Galaxy Based on Maser Kinematic Data

Abstract

Abstract A dynamic model of the Galaxy is constructed based on kinematic data for masers with trigonometric parallaxes. Maser data is used to compute the model potential in the Galactic plane. The potential is then generalized to three dimensions assuming the existence of a third quadratic integral of motion. The resulting Galactic model potential is of Stäckel’s type. The corresponding space density function is determined from Poisson’s equation.

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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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citations
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!
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