Addition of the Local Volume sample of galaxies from the FAST HI survey
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arXiv
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| Autores principales: | , , , |
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| Formato: | Preprint |
| Publicado: |
2024
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| _version_ | 1866914776556240896 |
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| author | Karachentsev, Igor D. Karachentseva, Valentina E. Kaisin, Serafim S. Zhang, Chuan-Peng |
| author_facet | Karachentsev, Igor D. Karachentseva, Valentina E. Kaisin, Serafim S. Zhang, Chuan-Peng |
| contents | {We report the discovery of 20 new dwarf galaxies in the Local Volume identified as optical counterparts to the Five-hundred-meter Aperture Spherical radio Telescope (FAST) All Sky HI Survey (FASHI) sources. The galaxies have a median stellar mass of $7.8\times 10^6~M_{\odot}$ and a median HI mass of $1.0\times 10^7~M_{\odot}$. Most of them are field galaxies, while three are probable members of the M 101 and M 106 groups. We also found seven FASHI radio sources to be probable dark HI clouds in nearby groups. Together with four other known HI clouds in the local groups, their mean-square radial velocity difference of 49~km~s$^{-1}$ with respect to the host galaxies yields an average total mass of ($2.7\pm1.0)\times10^{11}~M_{\odot}$ for these groups on the projected scale of 90 kpc. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2404_07636 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Addition of the Local Volume sample of galaxies from the FAST HI survey Karachentsev, Igor D. Karachentseva, Valentina E. Kaisin, Serafim S. Zhang, Chuan-Peng Astrophysics of Galaxies {We report the discovery of 20 new dwarf galaxies in the Local Volume identified as optical counterparts to the Five-hundred-meter Aperture Spherical radio Telescope (FAST) All Sky HI Survey (FASHI) sources. The galaxies have a median stellar mass of $7.8\times 10^6~M_{\odot}$ and a median HI mass of $1.0\times 10^7~M_{\odot}$. Most of them are field galaxies, while three are probable members of the M 101 and M 106 groups. We also found seven FASHI radio sources to be probable dark HI clouds in nearby groups. Together with four other known HI clouds in the local groups, their mean-square radial velocity difference of 49~km~s$^{-1}$ with respect to the host galaxies yields an average total mass of ($2.7\pm1.0)\times10^{11}~M_{\odot}$ for these groups on the projected scale of 90 kpc. |
| title | Addition of the Local Volume sample of galaxies from the FAST HI survey |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2404.07636 |