New HI observations Toward the NGC 5055 Galaxy Group with FAST

We report a new high-sensitivity HI mapping observation of the NGC 5055 galaxy group over an area of $1.^\circ5\times0.^\circ75$ with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). Our observation reveals that the warped H\,{\sc i} disk of NGC~5055 is more extended than what previously observed by WSRT, out to $ 23.'9$ (61.7 kpc). The total HI mass of NGC 5055 is determined to be $\rm\sim 1.1\times10^{10}\,M_\odot$. We identified three HI clouds with HI masses of the order of $\rm \sim 10^7\,M_\odot$ at the southeastern edge of the HI disk, as well as a candidate high-velocity cloud with an HI mass of $\rm (1.2\pm0.5) \times10^6\,M_\odot$ to the north of NGC 5055. The HI content of UGCA 337 is robustly detected for the first time by the FAST observations. It has a narrow HI linewidth of $W_{50}=17.4\pm3.8$ km s$^{-1}$ with a total \HI\ mass of ($\rm 3.5\pm0.3)\times10^6\,M_\odot$. Comparing the gas content and g-r color of UGCA 337 with typical low-mass dwarf galaxies, UGCA~337 appears relatively gas-poor despite its blue color. This suggests that UGCA 337 may have undergone gas stripping in the past. We also analyzed the possible origin of the diffuse HI clouds located at the outskirts of NGC 5055, and speculate that they might be the remnant features of a merger event in the past.