Pilot HI Survey of Planck Galactic Cold Clumps with FAST
Ningyu Tang, Di Li, Pei Zuo, Lei Qian, Tie Liu, Yuefang Wu, Marko, Kr\v{c}o, Mengting Liu, Youling Yue, Yan Zhu, Hongfei Liu, Dongjun Yu,, Jinghai Sun, Peng Jiang, Gaofeng Pan, Hui Li, Hengqian Gan, Rui Yao, Shu Liu,, and FAST Collaboration

TL;DR
This pilot survey using FAST observed 17 PGCCs to detect cold HI via HINSA, revealing insights into atomic-molecular transition, HI abundance, and cloud ages, with findings indicating depletion of cold HI in denser clouds.
Contribution
First FAST-based HI survey of PGCCs utilizing HINSA to analyze cold HI properties and cloud evolution, providing new data on atomic to molecular transition in cold clumps.
Findings
HINSA detected in 58% of PGCCs
HI abundance relative to total hydrogen is higher than previous surveys
Inverse correlation between HINSA abundance and total hydrogen column density in dense clouds
Abstract
We present a pilot HI survey of 17 Planck Galactic Cold Clumps (PGCCs) with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). HI Narrow Self-Absorption (HINSA) is an effective method to detect cold HI being mixed with molecular hydrogen H and improves our understanding of the atomic to molecular transition in the interstellar medium. HINSA was found in 58\% PGCCs that we observed. The column density of HINSA was found to have an intermediate correlation with that of CO, following . HI abundance relative to total hydrogen [HI]/[H] has an average value of , which is about 2.8 times of the average value of previous HINSA surveys toward molecular clouds. For clouds with total column density N cm, an inverse correlation between HINSA abundance…
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