activity
20182023
most citedA Q-band line survey towards Orion KL using the Tianma radio telescope

15 citations · 46 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2023

The first Ka-band (26.1-35 GHz) blind line survey towards Orion KL

Xunchuan Liu, Tie Liu, Zhiqiang Shen +30

We conducted a Ka-band (26.1--35 GHz) line survey towards Orion KL using the TianMa 65-m Radio Telescope (TMRT). It is the first blind line survey in the Ka band, and achieves a se…

astro-ph.GA202215 cited

A Q-band line survey towards Orion KL using the Tianma radio telescope

Xunchuan Liu, Tie Liu, Zhiqiang Shen +28

We have conducted a line survey towards Orion KL using the Q-band receiver of Tianma 65 m radio telescope (TMRT), covering 34.8--50 GHz with a velocity resolution between 0.79 km s…

astro-ph.GA20217 cited

Planck Galactic Cold Clumps at High Galactic Latitude-A Study with CO Lines

Fengwei Xu, Yuefang Wu, Tie Liu +28

Gas at high Galactic latitude is a relatively little-noticed component of the interstellar medium. In an effort to address this, forty-one Planck Galactic Cold Clumps at high Galac…

astro-ph.GA2020

Planck Galactic Cold Clumps in Two Regions: the First Quadrant and the Anti-Center Direction Region

Chao Zhang, Yuefang Wu, Xunchuan Liu +13

Sixty five Planck Galactic cold clumps (PGCCs) from the first quadrant (IQuad) and thirty nine of PGCCs from the Anti-Center direction region (ACent) were observed in CO, $^…

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,…