On the massive disks in low surface brightness galaxies

dc.contributor.author	Saburova, A.S.
dc.date.accessioned	2017-06-01T17:57:37Z
dc.date.available	2017-06-01T17:57:37Z
dc.date.issued	2011
dc.identifier.citation	On 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.isbn	987-966-439-367-3
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/118967
dc.description.abstract	On 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.sponsorship	I 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.language.iso	en	uk_UA
dc.publisher	Advances in astronomy and space physics	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.title	On the massive disks in low surface brightness galaxies	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA