2 citations · 2 across the 4 of their papers we have counts for
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FAST Observations of Filamentary and Compact H I Structure in a Magellanic Stream IV Field
Yuxin Xiao, Qingzheng Yu, Taotao Fang +3
The Magellanic Stream (MS) is believed to have formed from gas removed from the Large and Small Magellanic Clouds through tidal forces and hydrodynamic interactions with the Milky…
The Intrinsic Multiphase Gas--Black Hole Connection across Scales in IllustrisTNG
Xiaoxia Zhang, Taotao Fang, Shulan Yan +2
The relationship between supermassive black holes and the multiphase circumgalactic medium is central to understanding the co-evolution of galaxies and their central black holes. W…
The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk
Xiaochuan Jiang, Taotao Fang, Shulan Yan
The physical properties of Milky Way Mgii-bearing gas remain poorly constrained due to the saturation of the near-UV doublet. We utilize the weaker Mgii 1239, 1240 doublet from…
HI Gas and Star Formation in Major Galaxy Pairs from the FAST All-Sky HI Survey (FASHI)
Shulan Yan, Qingzheng Yu, Taotao Fang +6
Atomic hydrogen (HI) plays a fundamental role in fueling star formation in galaxies. However, the behavior of HI gas in interacting systems, particularly galaxy pairs, remains elus…