activity
20192021
most citedCarbon-Chain Molecules in Molecular Outflows and Lupus I Region--New Producing Region and New Forming Mechanism

14 citations · 35 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2021

Molecular Clouds in the Second Quadrant of the Milky Way Mid-plane from l10475 to l=11975 and b=525 to b=525

Yuehui Ma, Hongchi Wang, Chong Li +3

We have studied the properties of molecular clouds in the second quadrant of the Milky Way Mid-plane from l10475 to l11975 and b5$.\!\!^{\ci…

astro-ph.GA20203 cited

The Molecular Clouds associated with the H II Regions/Candidates between and

Chong Li, Hongchi Wang, Miaomiao Zhang +2

Using the PMO-13.7 m millimeter telescope at Delingha in China, we have conducted a large-scale simultaneous survey of CO, CO, and CO emission toward t…

astro-ph.GA20208 cited

A Cold and Diffuse Giant Molecular Filament in the Region of ,

Liang-Hao Lin, Hong-Chi Wang, Yang Su +2

Data of CO/CO/CO emission toward the Galactic plane region of to and to are available with the Milky…

astro-ph.GA2019

Assessing the Performance of Molecular Gas Clump Identification Algorithms

Chong Li, Hong-chi Wang, Yuan-wei Wu +2

The detection of clumps(cores) in molecular clouds is an important issue in sub-millimetre astronomy. However, the completeness of the identification and the accuracy of the return…

astro-ph.SR201914 cited

Carbon-Chain Molecules in Molecular Outflows and Lupus I Region--New Producing Region and New Forming Mechanism

Yuefang Wu, Xunchuan Liu, Xi Chen +18

Using the new equipment of the Shanghai Tian Ma Radio Telescope, we have searched for carbon-chain molecules (CCMs) towards five outflow sources and six Lupus I starless dust cores…

astro-ph.SR201910 cited

A particular carbon-chain-producing region: L1489 starless core

Yuefang Wu, Lianghao Lin, Xunchuan Liu +14

We detected carbon-chain molecules (CCMs) HC2n+1N (n=1-3) and C3S in Ku band as well as {high-energy excitation lines including C4H N=9-8, J=17/2-15/2, 19/2-17/2, and CH3CCH J=5-4,…