activity
20202023
most citedThe chemical structure of young high-mass star-forming clumps: (II) parsec-scale CO depletion and deuterium fraction of

29 citations · 78 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2023

Understanding the Kinetic Energy deposition within Molecular Clouds

Lixia Yuan, Ji Yang, Fujun Du +8

According to the structures traced by CO spectral lines within the CO molecular clouds (MCs), we investigate the contributions of their internal gas motions and relat…

astro-ph.GA2022★ 10 cited

A detailed temperature map of the archetypal protostellar shocks in L1157

S. Feng, H. B. Liu, P. Caselli +5

We present sensitive (1,1)--(7,7) line images from the Karl G. Jansky Very Large Array toward successive shocks, which are associated with the blueshifted outflow lobe d…

astro-ph.GA2022★ 17 cited

Unusually high HCO+/CO ratios in and outside supernova remnant W49B

Ping Zhou, Gao-Yuan Zhang, Xin Zhou +10

Galactic supernova remnants (SNRs) and their environments provide the nearest laboratories to study SN feedback. We performed molecular observations toward SNR W49B, the most lumin…

astro-ph.GA2021★ 22 cited

Physical and chemical structure of the Serpens filament -- fast formation and gravity-driven accretion

Y. Gong, A. Belloche, F. J. Du +5

The Serpens filament, a prominent elongated structure in a relatively nearby molecular cloud, is believed to be at an early evolutionary stage, so studying its physical and chemica…

astro-ph.GA2020★ 29 cited

The chemical structure of young high-mass star-forming clumps: (II) parsec-scale CO depletion and deuterium fraction of

S. Feng, D. Li, P. Caselli +19

The physical and chemical properties of cold and dense molecular clouds are key to understanding how stars form. Using the IRAM 30 m and NRO 45 m telescopes, we carried out a Multi…