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

40 papers

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.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★ 2 cited

Origins of the shocks in high-mass starless clump candidates

Feng-Yao Zhu, Junzhi Wang, Yaoting Yan +2

Shocks are abundant in star-forming regions, and are often related with star formation. In our previous observations toward 100 starless clump candidates (SCCs) in the Galaxy, a sa…

astro-ph.GA2023★ 7 cited

Spatial distributions and kinematics of shocked and ionized gas in M17

Feng-Yao Zhu, Junzhi Wang, Yaoting Yan +2

Massive stars are formed in molecular clouds, and produce H II regions when they evolve onto the main sequence. The expansion of H II region can both suppress and promote star form…

astro-ph.GA2023★ 4 cited

OO abundance ratio toward a sample of massive star forming regions with parallax distances

Chao Ou, Junzhi Wang, Siqi Zheng +3

The OO abundance ratio is, in principle, a powerful tool to estimate the relative contributions of massive stars and low- to intermediate-mass stars to the chemical…

astro-ph.GA2023★ 4 cited

Imaging Molecular Outflow in Massive Star-forming Regions with HNCO Lines

Jinjin Xie, Juan Li, Junzhi Wang +8

Protostellar outflows are considered a signpost of star formation. These outflows can cause shocks in the molecular gas and are typically traced by the line wings of certain molecu…