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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| Veröffentlicht in: | Advances in Astronomy and Space Physics |
|---|---|
| Datum: | 2011 |
| 1. Verfasser: | |
| Format: | Artikel |
| Sprache: | English |
| Veröffentlicht: |
Advances in astronomy and space physics
2011
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| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/118967 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Zitieren: | 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| id |
nasplib_isofts_kiev_ua-123456789-118967 |
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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 |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
On the massive disks in low surface brightness galaxies |
| spellingShingle |
On the massive disks in low surface brightness galaxies Saburova, A.S. |
| title_short |
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_sort |
on the massive disks in low surface brightness galaxies |
| author |
Saburova, A.S. |
| author_facet |
Saburova, A.S. |
| publishDate |
2011 |
| language |
English |
| container_title |
Advances in Astronomy and Space Physics |
| publisher |
Advances in astronomy and space physics |
| format |
Article |
| 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.
|
| isbn |
987-966-439-367-3 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/118967 |
| 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. |
| work_keys_str_mv |
AT saburovaas onthemassivedisksinlowsurfacebrightnessgalaxies |
| first_indexed |
2025-11-27T21:19:01Z |
| last_indexed |
2025-11-27T21:19:01Z |
| _version_ |
1850852841724313600 |