20 citations · 42 across the 7 of their papers we have counts for
7 papers
A FAST Survey of H I Absorption in Low-power Radio Sources
Yang Su, Qingzheng Yu, Taotao Fang +3
We conducted a HI 21cm absorption study of a sample of 147 nearby (z < 0.1) low-power radio sources with and $\log(P_{…
A Systematic Search for Gaseous Debris Disks in DESI Early Data Release White Dwarfs
Ziying Ma, Xiaoxia Zhang, Taotao Fang +5
Detecting gaseous debris disks around white dwarfs offers a unique window into the ultimate fate of planetary systems and the composition of accreted planetary material. Here we pr…
HI Content of Group Galaxies from the FAST All Sky HI Survey
Shulan Yan, Andrew Ma, Qingzheng Yu +3
We investigate the atomic gas (HI) content of galaxies in groups using early data from the FAST All Sky HI survey (FASHI). Taking advantage of FAST's blind, wide-area coverage and…
Tracing the Origins of Hot Halo Gas in Milky Way-Type Galaxies with SMUGGLE
Zhijie Zhang, Xiaoxia Zhang, Hui Li +8
Current galaxy formation models predict the existence of X-ray-emitting gaseous halos around Milky Way (MW)-type galaxies. To investigate properties of this coronal gas in MW-like…
Stellar Flyby Analysis for Spiral Arm Hosts with Gaia DR3
Linling Shuai, Bin B. Ren, Ruobing Dong +5
Scattered light imaging studies have detected nearly two dozen spiral arm systems in circumstellar disks, yet the formation mechanisms for most of them are still under debate. Alth…
An Empirical Determination of the Dependence of the Circumgalactic Mass Cooling Rate and Feedback Mass Loading Factor on Galactic Stellar Mass
Huanian Zhang, Dennis Zaritsky, Karen Pardos Olsen +9
Using our measurements of the H emission line flux originating in the cool (T K) gas that populates the halos of galaxies, we build a joint model to describe mass of…
Observing the Effects of Galaxy Interactions on the Circumgalactic Medium
Huanian Zhang, Taotao Fang, Dennis Zaritsky +3
We continue our empirical study of the emission line flux originating in the cool ( K) gas that populates the halos of galaxies and their environments. Specifically, we…