activity
20232026
most citedGravitationally Bound Gas Determines Star Formation in the Galaxy

8 citations · 30 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.GA2026

Anomalously high deuterium fractionation in a galactic translucent cloud: a challenge to chemical models

Gan Luo, Zhi-Yu Zhang, Thomas G. Bisbas +8

Deuterated (D-) species have long been proposed to diagnose the physical conditions and chemical evolution of cold dense molecular clouds. While deuterium fractionation has been ex…

astro-ph.GA2026

NO molecule in massive star forming regions

Shaomin Su, Junzhi Wang, Rui Luo +7

Context. Among diatomic molecules composed of the abundant elements C, N and O, NO has been detected far less than the well studied CN and CO, making it a crucial yet under-observe…

astro-ph.GA2026

The gas kinematics in 70 μm dark molecular clumps with ammonia

Chao Ou, Shanghuo Li, Junzhi Wang +5

We present the investigation of the gas kinematics and assess the evolutionary stages of dense cores embedded in four infrared dark clouds (IRDCs) using the NH(1,1) and NH(…

astro-ph.GA2026

Star Formation Drives Production of Low Energy Cosmic Rays

Ningyu Tang, Jiahao Liu, Di Li +18

For over a century, the origin of low-energy cosmic rays (LECRs), the dominant heaters and ionizers of dense interstellar gas, remains elusive owing to solar modulation and uncerta…

astro-ph.GA2026

The evolution of C4H and c-C3H2 in molecular cores

Yijia Liu, Junzhi Wang, Ningyu Tang +8

Linear C4H and cyclic c-C3H2, as small unsaturated hydrocarbons, are the key precursors to complex organic molecules and are critical components of the interstellar medium. We pres…

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

Torus feeding and outflow launching in the active nucleus of the Circinus galaxy

Wout M. Goesaert, Konrad R. W. Tristram, C. M. Violette Impellizzeri +4

Context: Most active galactic nuclei (AGN) are believed to be surrounded by a dusty molecular torus on the parsec scale which is often embedded within a larger circumnuclear disk (…

astro-ph.GA2025★ 1 cited

Scientific Objectives of the Xue-shan-mu-chang 15-meter Submillimeter Telescope

XSMT Project Collaboration Group, Yiping Ao, Jin Chang +48

Submillimeter astronomy is poised to revolutionize our understanding of the Universe by revealing cosmic phenomena hidden from optical and near-infrared observations, particularly…

astro-ph.GA2025★ 8 cited

Gravitationally Bound Gas Determines Star Formation in the Galaxy

Sihan Jiao, Jingwen Wu, Zhi-Yu Zhang +13

Stars form from molecular gas under complex conditions influenced by multiple competing physical mechanisms, such as gravity, turbulence, and magnetic fields. However, accurately i…

astro-ph.GA2025★ 1 cited

Physical Properties and HI-to-H2 Transition Across Taurus Linear Edge

Ningyu Tang, Feihang Miao, Gan Luo +5

Studying the atomic-to-molecular transition is essential for understanding the evolution of interstellar medium. The linear edge of Taurus molecular cloud, clearly identified in th…

astro-ph.GA2025★ 1 cited

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.GA2025★ 6 cited

Inadequate turbulent support in low-metallicity molecular clouds

Lingrui Lin, Zhi-Yu Zhang, Junzhi Wang +16

The dynamic properties of molecular clouds are set by the interplay of their self-gravity, turbulence, external pressure and magnetic fields. Extended surveys of Galactic molecular…

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.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.GA2024★ 2 cited

Spatial distribution of C4H and c-C3H2 in cold molecular cores

Yijia Liu, Junzhi Wang, Shu Liu +6

CH and -CH, as unsaturated hydrocarbon molecules, are important for forming large organic molecules in the interstellar medium. We present mapping observations of C$…

astro-ph.GA2024★ 2 cited

Dense Outflowing Molecular Gas in Massive Star-forming Regions

Yani Xu, Junzhi Wang, Shu Liu +6

Dense outflowing gas, traced by transitions of molecules with large dipole moment, is important for understanding mass loss and feedback of massive star formation. HCN 3-2 and HCO$…

astro-ph.GA2023★ 4 cited

Molecular deuterations in massive Starless Clump Candidates

Kai Yang, Junzhi Wang, Keping Qiu +1

Deuterated molecules are valuable probes for investigating the evolution and the kinematics in the earliest stages of star formation. In this study, we conduct a comprehensive inve…

astro-ph.GA2023

An improved method to measure and abundance ratios: revisiting CN isotopologues in the Galactic outer disk

Yichen Sun, Zhi-Yu Zhang, Junzhi Wang +7

The variations of elemental abundance and their ratios along the Galactocentric radius result from the chemical evolution of the Milky Way disks. The ratio in p…

astro-ph.GA2023★ 4 cited

Spatial distribution of NH2D in massive star-forming regions

Yuqiang Li, Junzhi Wang, Juan Li +4

To understand the relation between NHD and its physical environment, we mapped ortho-NHD at 85.9 GHz toward 24 Galactic late-stage massive star-forming…

astro-ph.GA2023

Tentative detection of cyanoformamide NCCONH2 in space

Juan Li, Donghui Quan, Junzhi Wang +12

The peptide-like molecules, cyanoformamide (NCCONH2), is the cyano (CN) derivative of formamide (NH2CHO). It is known to play a role in the synthesis of nucleic acid precursors und…

astro-ph.GA2023

Sulphur isotopes toward Sagittarius B2 extended envelope in the Galactic Center

Qingxu Li, Juan Li, Siqi Zheng +3

The isotopic ratios are good tools for probing the stellar nucleosynthesis and chemical evolution. We performed high-sensitivity mapping observations of the J=7-6 rotational transi…

astro-ph.GA2023

Mapping Observations of Peptide-like molecules around Sagittarius B2

Siqi Zheng, Juan Li, Junzhi Wang +7

Peptide-like molecule, which has a close connection with the origin of life, has been detected in universe. Mapping observations of HCONH and CHCONH, two simplest pepti…