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Tie Liu

15 papers here

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

author position
  • first author1
  • middle author10

Across the 11 of 15 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA11
  • astro-ph.SR4
ORCID 0000-0002-5286-2564
same name
  • Tie Liu — 92 papers, h 29
  • Tie Liu — 45 papers, h 8
  • Tie Liu — 24 papers, h 6
  • Tie Liu — 16 papers, h 4
  • Tie Liu — 10 papers, h 23
  • Tie Liu — 6 papers, h 4

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
20142025
most citedEvidence of high-mass star formation through multi-scale mass accretion in hub-filament-system clouds

55 citations · 263 across the 15 of their papers we have counts for

collaborators
Showing 2014Show all

4 papers · 1 filter

astro-ph.SR2014★ 44 cited

A feedback-driven bubble G24.136+00.436: a possible site of triggered star formation

Hong-Li Liu, Yuefang Wu, JinZeng Li +3

We present a multi-wavelength study of the IR bubble G24.136+00.436. The J=1-0 observations of 12CO, 13CO and C18O were carried out with the Purple Mountain Observat…

astro-ph.SR2014

Inflows in massive star formation regions

Yuefang Wu, Tie Liu, Shengli Qin

How high-mass stars form remains unclear currently. Calculation suggests that the radiation pressure of a forming star can halt spherical infall, preventing its further growth when…

astro-ph.SR2014

Follow-up observations toward Planck cold clumps with ground-based radio telescopes

Tie Liu, Yuefang Wu, Diego Mardones +26

The physical and chemical properties of prestellar cores, especially massive ones, are still far from being well understood due to the lack of a large sample. The low dust temperat…

astro-ph.SR2014★ 3 cited

A CO observation of the galactic methanol masers

Zhiyuan Ren, Yuefang Wu, Tie Liu +3

Context: We investigated the molecular gas associated with 6.7 GHz methanol masers throughout the Galaxy using a J=1-0 transition of the CO isotopologues. Methods:Using the 13.7-me…

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