activity
20042026
most citedInefficient Star Formation In Extremely Metal Poor Galaxies

210 citations · 2.2k across the 82 of their papers we have counts for

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Showing astro-ph.GAShow all

69 papers · 1 filter

astro-ph.GA2026

Constrain the Size of Broad Line Region in NGC 1068 Using Sub-millimeter Excess

Qi Guo, Junzhi Wang, Lingrui Lin +3

Constraining the size of broad-line region (BLR) close to the accretion disk in active galactic nuclei (AGNs) is key to understand the central engine and evolution of AGN. We propo…

astro-ph.GA2023★ 2 cited

Opacities of dense gas tracers in galactic massive star-forming regions

Shu Liu, Junzhi Wang, Fei Li +5

Optical depths of dense molecular gas are commonly used in Galactic and extragalactic studies to constrain the dense gas mass of the clouds or galaxies. The optical depths are ofte…

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…