SOME PECULIARITIES OF THE RADIAL GAS DISTRIBUTION IN GALACTIC DISC

This paper reports on the theoretical investigation of evolution of the Galaxy. The spiral arms and radial gas flows can be considered as some kind of indicators of the dynamical processes in the disc. Investigation the surface density of gas. The velocity profiles of radial gas flows were selecte...

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Main Author: M. V. Dzyubenko
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2017-04-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/98247
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author M. V. Dzyubenko
author_facet M. V. Dzyubenko
author_sort M. V. Dzyubenko
collection DOAJ
description This paper reports on the theoretical investigation of evolution of the Galaxy. The spiral arms and radial gas flows can be considered as some kind of indicators of the dynamical processes in the disc. Investigation the surface density of gas. The velocity profiles of radial gas flows were selected in such a way to have an agreement between the model predictions and observational data. The model with the radial gas flows gives the results that appear to be in the better agreement with the observations. The results of the model predictions differ significantly comparing to the case of the standard Galactic evolutionary model.
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spelling doaj.art-b558086183ac4430932d404f2b19564b2022-12-22T00:40:43ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152017-04-01180495110.18524/1810-4215.2005.18.9824798247SOME PECULIARITIES OF THE RADIAL GAS DISTRIBUTION IN GALACTIC DISCM. V. Dzyubenko0Department of Astronomy, Odessa National University, T.G.Shevchenko Park, Odessa 65014 UkraineThis paper reports on the theoretical investigation of evolution of the Galaxy. The spiral arms and radial gas flows can be considered as some kind of indicators of the dynamical processes in the disc. Investigation the surface density of gas. The velocity profiles of radial gas flows were selected in such a way to have an agreement between the model predictions and observational data. The model with the radial gas flows gives the results that appear to be in the better agreement with the observations. The results of the model predictions differ significantly comparing to the case of the standard Galactic evolutionary model.http://oap.onu.edu.ua/article/view/98247
spellingShingle M. V. Dzyubenko
SOME PECULIARITIES OF THE RADIAL GAS DISTRIBUTION IN GALACTIC DISC
Odessa Astronomical Publications
title SOME PECULIARITIES OF THE RADIAL GAS DISTRIBUTION IN GALACTIC DISC
title_full SOME PECULIARITIES OF THE RADIAL GAS DISTRIBUTION IN GALACTIC DISC
title_fullStr SOME PECULIARITIES OF THE RADIAL GAS DISTRIBUTION IN GALACTIC DISC
title_full_unstemmed SOME PECULIARITIES OF THE RADIAL GAS DISTRIBUTION IN GALACTIC DISC
title_short SOME PECULIARITIES OF THE RADIAL GAS DISTRIBUTION IN GALACTIC DISC
title_sort some peculiarities of the radial gas distribution in galactic disc
url http://oap.onu.edu.ua/article/view/98247
work_keys_str_mv AT mvdzyubenko somepeculiaritiesoftheradialgasdistributioningalacticdisc