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- W3217162776 abstract "We present results from deep HI and optical imaging of AGC 229101, an unusual HI source detected at v$_{rm helio}$ = 7116 km/s in the ALFALFA survey. Initially classified as a candidate dark source because it lacks a clear optical counterpart in SDSS or DSS2 imaging, AGC 229101 has $10^{9.31pm0.05}$ solar masses of HI, but an HI line width of only 43$pm$9 km/s. Low resolution WSRT imaging and higher resolution VLA B-array imaging show that the source is significantly elongated, stretching over a projected length of ~80 kpc. The HI imaging resolves the source into two parts of roughly equal mass. WIYN pODI optical imaging reveals a faint, blue optical counterpart coincident with the northern portion of the HI. The peak surface brightness of the optical source is only $mu_{g}$ = 26.6 mag arcsec$^{-2}$, well below the typical cutoff that defines the isophotal edge of a galaxy, and its estimated stellar mass is only $10^{7.32pm0.33}$ solar masses, yielding an overall neutral gas-to-stellar mass ratio of M$_{rm HI}$/M$_*=$~98$_{+111}atop^{-52}$. We demonstrate the extreme nature of this object by comparing its properties to those of other HI-rich sources in ALFALFA and the literature. We also explore potential scenarios that might explain the existence of AGC~229101, including a tidal encounter with neighboring objects and a merger of two dark HI clouds." @default.
- W3217162776 created "2021-12-06" @default.
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- W3217162776 date "2021-12-01" @default.
- W3217162776 modified "2023-09-27" @default.
- W3217162776 title "The ALFALFA Almost Dark Galaxy AGC 229101: A 2 Billion Solar Mass H i Cloud with a Very Low Surface Brightness Optical Counterpart" @default.
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- W3217162776 doi "https://doi.org/10.3847/1538-3881/ac2a38" @default.
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