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Junzhi Wang

23 papers hereh-index 327 citations31 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author23

Across the 23 of 23 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA22
  • astro-ph.SR1
same name
  • Junzhi Wang — 83 papers, h 21
  • Junzhi Wang — 9 papers, h 3
  • Junzhi Wang — 5 papers, h 1
  • Junzhi Wang — 4 papers, h 1
  • Junzhi Wang — 2 papers, h 2
  • Junzhi Wang — 2 papers, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

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
Showing 2024Show all

4 papers · 1 filter

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 NH3​ in massive star-forming regions

Yuqiang Li, Junzhi Wang, Juan Li +6

Deuteration is sensitive to environmental conditions in star-forming regions. To investigate NH2​D chemistry, we compared the spatial distribution of ortho-NH2​D $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

C4​H and c-C3​H2​, 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$…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.