On the massive disks in low surface brightness galaxies
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 t...
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| Published in: | Advances in Astronomy and Space Physics |
|---|---|
| Date: | 2011 |
| Main Author: | |
| Format: | Article |
| Language: | English |
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Advances in astronomy and space physics
2011
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| Online Access: | https://nasplib.isofts.kiev.ua/handle/123456789/118967 |
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| Journal Title: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Cite this: | 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. |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine| _version_ | 1862599076998021120 |
|---|---|
| author | Saburova, A.S. |
| author_facet | Saburova, A.S. |
| citation_txt | 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. |
| collection | DSpace DC |
| container_title | Advances in Astronomy and Space Physics |
| description | 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.
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| first_indexed | 2025-11-27T21:19:01Z |
| format | Article |
| fulltext | |
| id | nasplib_isofts_kiev_ua-123456789-118967 |
| institution | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| isbn | 987-966-439-367-3 |
| language | English |
| last_indexed | 2025-11-27T21:19:01Z |
| publishDate | 2011 |
| publisher | Advances in astronomy and space physics |
| record_format | dspace |
| spelling | Saburova, A.S. 2017-06-01T17:57:37Z 2017-06-01T17:57:37Z 2011 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. 987-966-439-367-3 https://nasplib.isofts.kiev.ua/handle/123456789/118967 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. 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. en Advances in astronomy and space physics Advances in Astronomy and Space Physics On the massive disks in low surface brightness galaxies Article published earlier |
| spellingShingle | On the massive disks in low surface brightness galaxies Saburova, A.S. |
| title | On the massive disks in low surface brightness galaxies |
| title_full | On the massive disks in low surface brightness galaxies |
| title_fullStr | On the massive disks in low surface brightness galaxies |
| title_full_unstemmed | On the massive disks in low surface brightness galaxies |
| title_short | On the massive disks in low surface brightness galaxies |
| title_sort | on the massive disks in low surface brightness galaxies |
| url | https://nasplib.isofts.kiev.ua/handle/123456789/118967 |
| work_keys_str_mv | AT saburovaas onthemassivedisksinlowsurfacebrightnessgalaxies |