activity
20232026
collaborators

5 papers

astro-ph.GA2026

CH3CCH as a thermometer in warm molecular gas

Yuqiang Li, Junzhi Wang, Juan Li +9

Kinetic temperature is a fundamental parameter in molecular clouds. Symmetric top molecules, such as NH and CHCCH, are often used as thermometers. However, at high temperat…

astro-ph.GA2025

Widespread Hot Molecular Gas Heated by Shear-induced Turbulence in the Galactic Center

Juan Li, Junzhi Wang, Zhiqiang Shen +13

We observed NH3 metastable inversion lines from (3, 3) to (18, 18) toward G0.66-0.13 in the Galactic center with the Shanghai Tianma 65m radio telescope and Yebes 40 m telescope. H…

astro-ph.GA2025

NN abundance ratio toward massive star-forming regions with different Galactic distances

Chang Ruan, Junzhi Wang, Chao Ou +2

The abundance ratio of NN is, in principle, a powerful tool for tracing stellar nucleosynthesis. This work aims to measure and analyze (N/N)($^…

astro-ph.GA2024

The deuterium fractionation of NH in massive star-forming regions

Yuqiang Li, Junzhi Wang, Juan Li +6

Deuteration is sensitive to environmental conditions in star-forming regions. To investigate NHD chemistry, we compared the spatial distribution of ortho-NHD $1_{11}^s-1_{0…

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…