Optical identification of the FASHI sources: toward the extended Local Volume
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arXiv
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| Auteurs principaux: | , , , , , |
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| Format: | Preprint |
| Publié: |
2026
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| _version_ | 1866908951548788736 |
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| author | Nazarova, Aleksandra E. Makarov, Dmitry I. Karachentsev, Igor D. Zhang, Chuan-Peng Chazov, Maksim I. Zhu, Ming |
| author_facet | Nazarova, Aleksandra E. Makarov, Dmitry I. Karachentsev, Igor D. Zhang, Chuan-Peng Chazov, Maksim I. Zhu, Ming |
| contents | We extracted a list of 662 nearby (within $\sim16$ Mpc) HI-detection sources from the Five-hundred-meter Aperture Spherical radio Telescope (FAST) All Sky HI Survey (FASHI) and made a visual identification of them with optical counterpart. This inspection led to the discovery of 71 new dwarf galaxies. All of them are dwarf irregular galaxies with ongoing star formation. They are characterized by the following median parameters: visual magnitude of $g=17.8$ mag and color $(g-r)=0.29$ mag, HI-flux $S_\mathrm{HI}=718$ mJy km/s, HI-mass $M_\mathrm{HI}=3.7\times10^7$ $M_\odot$, as well as the HI line-width of $W_{50}=37$ km/s. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2604_09082 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Optical identification of the FASHI sources: toward the extended Local Volume Nazarova, Aleksandra E. Makarov, Dmitry I. Karachentsev, Igor D. Zhang, Chuan-Peng Chazov, Maksim I. Zhu, Ming Astrophysics of Galaxies We extracted a list of 662 nearby (within $\sim16$ Mpc) HI-detection sources from the Five-hundred-meter Aperture Spherical radio Telescope (FAST) All Sky HI Survey (FASHI) and made a visual identification of them with optical counterpart. This inspection led to the discovery of 71 new dwarf galaxies. All of them are dwarf irregular galaxies with ongoing star formation. They are characterized by the following median parameters: visual magnitude of $g=17.8$ mag and color $(g-r)=0.29$ mag, HI-flux $S_\mathrm{HI}=718$ mJy km/s, HI-mass $M_\mathrm{HI}=3.7\times10^7$ $M_\odot$, as well as the HI line-width of $W_{50}=37$ km/s. |
| title | Optical identification of the FASHI sources: toward the extended Local Volume |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2604.09082 |