More Local Volume dwarf galaxy candidates
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arXiv
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| Format: | Preprint |
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2025
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| _version_ | 1866909455892873216 |
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| author | Karachentsev, I. D. Karachentseva, V. E. Vladimirova, K. V. Kozyrev, K. A. |
| author_facet | Karachentsev, I. D. Karachentseva, V. E. Vladimirova, K. V. Kozyrev, K. A. |
| contents | We present the results of searching for new dwarf galaxies in the Local Volume. We found 40 satellite candidates in the double-virial-radius regions of 20 Milky Way-like and LMC-like galaxies in the southern sky using DESI Legacy Imaging Surveys, 10 of which were known but not clearly associated with the Local Volume previously. Among the 40 satellite candidates, 8 are supposed members of the NGC6744 group and 13 are located in the vicinity of the Sombrero galaxy. Based on seven companions to the giant spiral galaxy NGC\,6744 with measured radial velocities, we estimate that the total mass of the group is $M_T = (1.88\pm0.71)\times 10^{12} M_{\odot}$ and the total mass-to-K-luminosity ratio $M_T/L_K = (16.1\pm6.0) M_{\odot}/L_{\odot}$. We reproduce a distribution of 68 early- and late-type galaxies in the Local Volume situated around the Sombrero, noting their strong morphological segregation and also the presence of a foreground diffuse association of dwarf galaxies at 8 degrees to SE from the Sombrero. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2501_07912 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | More Local Volume dwarf galaxy candidates Karachentsev, I. D. Karachentseva, V. E. Vladimirova, K. V. Kozyrev, K. A. Astrophysics of Galaxies We present the results of searching for new dwarf galaxies in the Local Volume. We found 40 satellite candidates in the double-virial-radius regions of 20 Milky Way-like and LMC-like galaxies in the southern sky using DESI Legacy Imaging Surveys, 10 of which were known but not clearly associated with the Local Volume previously. Among the 40 satellite candidates, 8 are supposed members of the NGC6744 group and 13 are located in the vicinity of the Sombrero galaxy. Based on seven companions to the giant spiral galaxy NGC\,6744 with measured radial velocities, we estimate that the total mass of the group is $M_T = (1.88\pm0.71)\times 10^{12} M_{\odot}$ and the total mass-to-K-luminosity ratio $M_T/L_K = (16.1\pm6.0) M_{\odot}/L_{\odot}$. We reproduce a distribution of 68 early- and late-type galaxies in the Local Volume situated around the Sombrero, noting their strong morphological segregation and also the presence of a foreground diffuse association of dwarf galaxies at 8 degrees to SE from the Sombrero. |
| title | More Local Volume dwarf galaxy candidates |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2501.07912 |