activity
19962024
most citedThe Star Formation Rate and Dense Molecular Gas in Galaxies

1k citations · 7k across the 138 of their papers we have counts for

collaborators

137 papers

astro-ph.GA2024★ 5 cited

CO Observations of Early-mid Stage Major Mergers in the MaNGA Survey

Qingzheng Yu, Taotao Fang, Cong Kevin Xu +5

We present a study of the molecular gas in early-mid stage major-mergers, with a sample of 43 major-merger galaxy pairs selected from the Mapping Nearby Galaxies at Apache Point Ob…

astro-ph.GA2023★ 16 cited

SUNRISE: The rich molecular inventory of high-redshift dusty galaxies revealed by broadband spectral line surveys

Chentao Yang, Alain Omont, Sergio Martín +21

Understanding the nature of high- dusty galaxies requires a comprehensive view of their ISM and molecular complexity. However, the molecular ISM at high- is commonly studied…

astro-ph.GA2023★ 10 cited

Dense gas and star formation in the Outer Milky Way

Jonathan Braine, Yan Sun, Yoshito Shimajiri +5

We present maps and spectra of the HCN(1-0) and HCO(1-0) lines in the extreme outer Galaxy, at galactocentric radii between 14 and 22 kpc, with the 13.7 meter Delingha telescop…

astro-ph.SR2023★ 8 cited

Variability of Young Stellar Objects in the Perseus Molecular Cloud

Xiao-Long Wang, Min Fang, Gregory J. Herczeg +5

We present an analysis of 288 young stellar objects (YSOs) in the Perseus Molecular Cloud that have well defined and -band lightcurves from the Zwicky Transient Facility. Of…

astro-ph.GA2022★ 2 cited

Non-detection of Broad Hydrogen Radio Recombination Lines in Circinus Galaxy

Junzhi Wang, Yong Shi, Zhi-Yu Zhang +5

The line widths of broad line regions (BLRs) of AGNs are key parameters for understanding the central super massive black holes (SMBHs). However, due to obscuration from dusty toru…

astro-ph.GA2022★ 1 cited

A scaling relation in [C II]-detected galaxies and its likely application in cosmology

Y. Wu, Yu Gao, Jun-Feng Wang

We identify and investigate a possible correlation between the luminosity and linewidth in the -detected galaxies. Observationally, the strength of t…