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Odessa Astronomical Publications
Article . 2014
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THE ASYMMETRIC DRIFT AND THE ROTATION CURVE OF THE GALAXY

descriptionPublicationkeyboard_double_arrow_right Article 01 Oct 2014 English Publisher:Odessa I. I. Mechnykov National UniversityJournal:Odessa Astronomical Publications (issn: 1810-4215, Copyright policy )
Authors: O. Golubov;

THE ASYMMETRIC DRIFT AND THE ROTATION CURVE OF THE GALAXY

Abstract

Asymmetric drift in the solar neighbourhood is studied by the means of the RAVE data. The asymmetric drift correction is applied to the SDSS data to measure the rotation curve of the Milky Way in the extended solar neighbourhood. The rotation curve is flat between7 and 10 kpc. Via fitting this flat rotation curve, and the inner rotation curve determined through tangent point method, density model of the Milky Way is constructed.

Keywords

galaxy disk, Astronomy, QB1-991, galaxy dynamics

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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!
0
Average
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