activity
20092024
most citedATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- I. Survey description and a first look at G9.62+0.19

112 citations · 761 across the 40 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2024★ 1 cited

3 mm Spectroscopic Observations of Massive Star-Forming Regions with IRAM 30-m

Xuefang Xu, Junzhi Wang, Qian Gou +6

Broadband spectroscopic observations with high sensitivity provide an unbiased way to detect emissions of molecules in space. We present deep observations from ~ 105.8 GHz to 113.6…

astro-ph.SR2019★ 28 cited

Mapping Observations of complex organic molecules around Sagittarius B2 with ARO 12m telescope

Juan Li, Junzhi Wang, Haihua Qiao +10

We performed high-sensitivity mapping observations of several complex organic molecules around Sagittarius B2 with ARO 12m telescope at 3-mm wavelength. Based on their spatial dist…

astro-ph.SR2019★ 14 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.SR2019★ 10 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,…

astro-ph.SR2017★ 19 cited

A spectral line survey of IRC +10216 between 13.3 and 18.5 GHz

Xiao-Yan Zhang, Qing-Feng Zhu, Juan Li +3

A spectral line survey of IRC +10216 between 13.3 and 18.5 GHz is carried out using the Shanghai Tian Ma 65 m Radio Telescope (TMRT-65m) with a sensitivity of < 7 mK. Thirty-five s…

astro-ph.SR2015★ 11 cited

SMA observations of C2H in High-Mass Star Forming Regions

Xue-Jian Jiang, Hauyu Baobab Liu, Qizhou Zhang +5

CH is a representative hydrocarbon that is abundant and ubiquitous in the interstellar medium (ISM). To study its chemical properties, we present Submillimeter Array (SMA) obse…