On the massive disks in low surface brightness galaxies

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dc.contributor.authorSaburova, A.S.
dc.date.accessioned2017-06-01T17:57:37Z
dc.date.available2017-06-01T17:57:37Z
dc.date.issued2011
dc.description.abstractOn the example of four low surface brightness galaxies we demonstrate that the mass-to-light ratio of their disks may be found from the condition of marginal gravitational stability. In this case their surface densities and halo/disk mass ratios appear to be rather typical for normal galaxies, and this does not conflict with their rotation curves.uk_UA
dc.description.sponsorshipI thank A. V. Zasov for the initiating this work and for helpful discussions. I also want to thank O. V. Abramova for carrying out the calculations of the thicknesses of stellar disks in the gravitational potential of a dark halo.uk_UA
dc.identifier.citationOn the massive disks in low surface brightness galaxies / A.S. Saburova // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 19-22. — Бібліогр.: 8 назв. — англ.uk_UA
dc.identifier.isbn987-966-439-367-3
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/118967
dc.language.isoenuk_UA
dc.publisherAdvances in astronomy and space physicsuk_UA
dc.relation.ispartofAdvances in Astronomy and Space Physics
dc.statuspublished earlieruk_UA
dc.titleOn the massive disks in low surface brightness galaxiesuk_UA
dc.typeArticleuk_UA

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Advances in Astronomy and Space Physics, 2011, вип. 1-2