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| Main Authors: | , , , , , , , , , , , , , |
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| Format: | Preprint |
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2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2502.01727 |
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| _version_ | 1866915135549865984 |
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| author | Arabsalmani, Maryam Roychowdhury, Sambit Schneider, Benjamin Springel, Volker Floc'h, Emeric Le Bournaud, Frederic Burkert, Andreas Cuillandre, Jean-Charles Duc, Pierre-Alain Emsellem, Eric Galárraga-Espinosa, Daniela Pian, Elena Renaud, Florent Zwaan, Martin A. |
| author_facet | Arabsalmani, Maryam Roychowdhury, Sambit Schneider, Benjamin Springel, Volker Floc'h, Emeric Le Bournaud, Frederic Burkert, Andreas Cuillandre, Jean-Charles Duc, Pierre-Alain Emsellem, Eric Galárraga-Espinosa, Daniela Pian, Elena Renaud, Florent Zwaan, Martin A. |
| contents | We identify a chain of galaxies along an almost straight line in the nearby Universe with a projected length of ~5 Mpc. The galaxies are distributed within projected distances of only 7-105 kpc from the axis of the identified filament. They have redshifts in a very small range of z=0.0361-0.0370 so that their radial velocities are consistent with galaxy proper motions. The filament galaxies are mainly star-forming and have stellar masses in a range of $\rm 10^{9.1}-10^{10.7}\,M_{\odot}$. We search for systems with similar geometrical properties in the full-sky mock galaxy catalogue of the MillenniumTNG simulations and find that although such straight filaments are unusual and rare, they are predicted by $Λ$CDM simulations (4% incidence). We study the cold HI gas in a 1.3 Mpc section of the filament through HI-21cm emission line observations and detect eleven HI sources, many more than expected from the HI mass function in a similar volume. They have HI masses $\rm 10^{8.5}-10^{9.5}\,M_{\odot}$ and are mostly within ~120 kpc projected distance from the filament axis. None of these HI sources has a confirmed optical counterpart. Their darkness together with their large HI-21cm line-widths indicate that they contain gas that might not yet be virialized. These clouds must be marking the peaks of the dark matter and HI distributions over large scales within the filament. The presence of such gas clouds around the filament spines is predicted by simulations, but this is the first time that the existence of such clouds in a filament is observationally confirmed. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2502_01727 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Pearls on a string: Dark and bright galaxies on a strikingly straight and narrow filament Arabsalmani, Maryam Roychowdhury, Sambit Schneider, Benjamin Springel, Volker Floc'h, Emeric Le Bournaud, Frederic Burkert, Andreas Cuillandre, Jean-Charles Duc, Pierre-Alain Emsellem, Eric Galárraga-Espinosa, Daniela Pian, Elena Renaud, Florent Zwaan, Martin A. Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena We identify a chain of galaxies along an almost straight line in the nearby Universe with a projected length of ~5 Mpc. The galaxies are distributed within projected distances of only 7-105 kpc from the axis of the identified filament. They have redshifts in a very small range of z=0.0361-0.0370 so that their radial velocities are consistent with galaxy proper motions. The filament galaxies are mainly star-forming and have stellar masses in a range of $\rm 10^{9.1}-10^{10.7}\,M_{\odot}$. We search for systems with similar geometrical properties in the full-sky mock galaxy catalogue of the MillenniumTNG simulations and find that although such straight filaments are unusual and rare, they are predicted by $Λ$CDM simulations (4% incidence). We study the cold HI gas in a 1.3 Mpc section of the filament through HI-21cm emission line observations and detect eleven HI sources, many more than expected from the HI mass function in a similar volume. They have HI masses $\rm 10^{8.5}-10^{9.5}\,M_{\odot}$ and are mostly within ~120 kpc projected distance from the filament axis. None of these HI sources has a confirmed optical counterpart. Their darkness together with their large HI-21cm line-widths indicate that they contain gas that might not yet be virialized. These clouds must be marking the peaks of the dark matter and HI distributions over large scales within the filament. The presence of such gas clouds around the filament spines is predicted by simulations, but this is the first time that the existence of such clouds in a filament is observationally confirmed. |
| title | Pearls on a string: Dark and bright galaxies on a strikingly straight and narrow filament |
| topic | Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2502.01727 |