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researcher

S. Liu

4 papers hereh-index 4104 citations7 works total

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

author position
  • middle author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.GA2
same name
  • S. Liu — 309 papers, h 51
  • S. Liu — 259 papers
  • S. Liu — 224 papers, h 17
  • S. Liu — 142 papers, h 5
  • S. Liu — 96 papers
  • S. Liu — 52 papers, h 8

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
20042024
most citedMapping the Outflow from G5.89-0.39 in SiO(5-4)

34 citations · 78 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2024★ 3 cited

Study of the high-mass star-forming region S255IR at various scales

I. I. Zinchenko, S. -Y. Liu, D. K. Ojha +2

The S255IR-SMA1 core contains the protostar NIRS3 with a mass of ∼20 M⊙​. Several years ago, the first burst of luminosity for massive protostars, caused by an episodic…

astro-ph.GA2020★ 29 cited

The chemical structure of young high-mass star-forming clumps: (II) parsec-scale CO depletion and deuterium fraction of HCO+

S. Feng, D. Li, P. Caselli +19

The physical and chemical properties of cold and dense molecular clouds are key to understanding how stars form. Using the IRAM 30 m and NRO 45 m telescopes, we carried out a Multi…

astro-ph2004★ 34 cited

Mapping the Outflow from G5.89-0.39 in SiO(5-4)

P. K. Sollins, T. R. Hunter, J. Battat +9

We have mapped the ultracompact HII region, G5.89-0.39, and its molecular surroundings with the Submillimeter Array at 2".8 x 1".8 angular resolution in 1.3 mm continuum, SiO(5-4),…

astro-ph2004★ 12 cited

Submillimeter Array Observations of CS J=14--13 Emission from the Evolved Star IRC+10216

K. H. Young, T. R. Hunter, D. J. Wilner +1

We present imaging observations of the evolved star IRC+10216 in the CS J=14--13 line at 685.4 GHz and associated submillimeter continuum at about 2'' resolution made with the part…

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