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researcher

Xing Lu

75 papers hereh-index 241.7k citations86 works total

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

author position
  • first author8
  • middle author52
  • last author1

Across the 61 of 75 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA71
  • astro-ph.SR3
  • astro-ph.IM1
same name
  • Xing Lu — 29 papers, h 6
  • Xing Lu — 11 papers, h 4
  • Xing Lu — 6 papers, h 1
  • Xing Lu — 4 papers, h 0
  • Xing Lu — 3 papers
  • Xing Lu — 2 papers, h 7

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
20142026
most citedThe ALMA Survey of 70 μm dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

207 citations · 2.6k across the 74 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2026★ 5 cited

Digging into the Interior of Hot Cores with ALMA (DIHCA). VII. Disk candidates around high-mass stars and evidence of anisotropic infall

Fernando A. Olguin, Patricio Sanhueza, Yoko Oya +19

We study the kinematics of condensations in 30 fields forming high-mass stars with ALMA at a high-resolution of ~0.08'' on average (~230 au). The presence of disks is important for…

astro-ph.SR2024

Filamentary Network and Magnetic Field Structures Revealed with BISTRO in the High-Mass Star-Forming Region NGC2264 : Global Properties and Local Magnetogravitational Configurations

Jia-Wei Wang, Patrick M. Koch, Seamus D. Clarke +154

We report 850 μm continuum polarization observations toward the filamentary high-mass star-forming region NGC 2264, taken as part of the B-fields In STar forming Regions Observat…

astro-ph.SR2015★ 191 cited

Fragmentation of Molecular Clumps and Formation of Protocluster

Qizhou Zhang, Ke Wang, Xing Lu +1

Sufficiently massive clumps of molecular gas collapse under self-gravity and fragment to spawn a cluster of stars that have a range of masses. We investigate observationally the ea…

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