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researcher

Shu Liu

4 papers here

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

author position
  • first author1
  • middle author1
  • last author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
ORCID 0000-0001-6016-5550
same name
  • Shu Liu — 24 papers
  • Shu Liu — 12 papers, h 5
  • Shu Liu — 8 papers, h 60
  • Shu Liu — 6 papers, h 9
  • Shu Liu — 6 papers
  • Shu Liu — 4 papers

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

most citedProperties of dense molecular gas along the major axis of M 82

6 citations · 18 across the 4 of their papers we have counts for

collaborators

4 papers

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★ 6 cited

Protonated hydrogen cyanide as a tracer of pristine molecular gas

Y. Gong, F. J. Du, C. Henkel +11

Protonated hydrogen cyanide, HCNH+, plays a fundamental role in astrochemistry because it is an intermediary in gas-phase ion-neutral reactions within cold molecular clouds. H…

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…

astro-ph.GA2022★ 6 cited

Properties of dense molecular gas along the major axis of M 82

Fei Li, Zhi-Yu Zhang, Junzhi Wang +6

Dense gas is important for galaxy evolution and star formation. Optically-thin dense-gas tracers, such as isotopologues of HCN, HCO+, etc., are very helpful to diagnose excitation…

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