activity
20202026
most citedThe atomic gas of star-forming galaxies at z0.05 as revealed by the Five-hundred-meter Aperture Spherical Radio Telescope

10 citations · 15 across the 5 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2026

A Morphological Identification and Study of Radio Galaxies from LoTSS DR2. III. The Multiwavelength Analysis of Winged Radio Galaxies

Soumen Kumar Bera, Taotao Fang, Magdalena Kunert-Bajraszewska +5

We present a multiwavelength follow-up study of 621 winged radio galaxies (WRGs) recently identified from LoTSS DR2, constituting the largest statistically significant samples of X…

astro-ph.GA2026

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…

astro-ph.GA2024

Close Major-merger Pairs at : Star-forming Galaxies with Pseudobulges

Chuan He, Cong Kevin Xu, Ute Lisenfeld +5

We present a study of star-forming galaxies (SFGs) with pseudobulges (bulges with Sérsic index ) in a local close major-merger galaxy pair sample (H-KPAIR). With data fr…

astro-ph.GA2023

Deep HI Mapping of Stephan's Quintet and Its Neighborhood

Cheng Cheng, Cong Kevin Xu, P. N. Appleton +8

We carried out deep mapping observations of the atomic hydrogen (HI) 21 cm line emission in a field centered on the famous galaxy group Stephan's Quintet (SQ), using the Five-hundr…

astro-ph.GA20215 cited

Searching for low-redshift faint galaxies with MMT/Hectospec

Cheng Cheng, Jia-Sheng Huang, Christopher N. A. Willmer +20

We present redshifts for 2753 low-redshift galaxies between with 18 22 obtained with Hectospec at the Multi-Mirror Telesco…

astro-ph.GA2020

UV and NIR size of the HI selected low surface brightness galaxies

Cheng Cheng, Wei Du, Cong Kevin Xu +10

How does the low surface brightness galaxies (LSBGs) form stars and assemble the stellar mass is one of the most important questions to understand the LSBG population. We select a…