Simulations find that tidal dwarf galaxies form and persist in galaxy clusters under moderate stellar feedback across all relevant viscosities, supporting their identification as stripped remnants matching multiple observed dwarf galaxy classes.
FAST and Dark: A catalogue of Dark Galaxy Candidates within 50 Mpc
2 Pith papers cite this work. Polarity classification is still indexing.
abstract
Using the first data release of the Five-hundred-meter Aperture Spherical radio Telescope (FAST) All-Sky HI survey (FASHI), we compile a catalogue of 70 dark galaxy candidates (DGCs) within 50 Mpc. We select DGCs without an identified optical counterpart at a limiting g-band magnitude of ~ 28 mag arcsec^-2 in the DESI Legacy Survey, using both automatic cross-checking with optical catalogues and visual inspection of the colour images. After validating our DGCs, excluding potential spurious detections, issues in the registered position of the HI sources, and possible Radio Frequency Interferences (RFIs), we analyse their distribution over the surveyed sky, HI mass, linewidths, and inferred distance. They appear evenly distributed across the surveyed area, with no apparent bias to isolation. We did not find any DGC within the Local Volume (11 Mpc) in the sky surveyed by this first release of FASHI. We compare the observed properties of DGCs with those of galaxies with optical counterparts, finding that DGCs tend to have higher linewidths for a given HI mass. We discuss our DGCs in light of theoretical works, and compare them with other observational samples from previous HI surveys. This work presents a catalogue of dark galaxy candidates, which can serve as a basis for follow-up studies.
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Comparisons of three cosmological simulations show HI-rich failed halos occupy different mass regimes and predict that more can be discovered locally in HI-poor environments rather than at high redshift.
citing papers explorer
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Merge and Strip II: Imprint of galaxy formation physics and viscosity on baryon-dominated dwarf galaxies
Simulations find that tidal dwarf galaxies form and persist in galaxy clusters under moderate stellar feedback across all relevant viscosities, supporting their identification as stripped remnants matching multiple observed dwarf galaxy classes.
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Beyond Cloud-9: The case for discovering more HI-rich failed halos
Comparisons of three cosmological simulations show HI-rich failed halos occupy different mass regimes and predict that more can be discovered locally in HI-poor environments rather than at high redshift.