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researcher

D. Li

4 papers hereh-index 28 citations5 works total

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

author position
  • middle author4

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

fields
  • astro-ph.GA4
same name
  • D. Li — 150 papers, h 5
  • D. Li — 56 papers, h 47
  • D. Li — 33 papers, h 11
  • D. Li — 29 papers
  • D. Li — 7 papers, h 6
  • D. Li — 7 papers, h 5

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

collaborators
Showing astro-ph.GAShow all

4 papers · 1 filter

astro-ph.GA2026

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde VI. The photodissociation region M17SW

X. Zhao, X. D. Tang, C. Henkel +20

The kinetic temperature structure of the photodissociation region M17SW was mapped using the IRAM 30 m telescope. This mapping employed the para-H2CO triplet (J(KaKc) = 303-202, 32…

astro-ph.GA2026

Molecular Clouds at the Edge of the Galaxy II. Physical properties and scaling relations

C. S. Luo, X. D. Tang, C. Henkel +22

The outer Galaxy presents an optimal setting for investigating molecular clouds and star formation in environments with low metallicity. A total of 72 Galactic edge clouds were sur…

astro-ph.GA2024

Dynamic Massive Star Formation: Radio Flux Variability in UCHII Regions

A. Y. Yang, M. A. Thompson, J. S. Urquhart +7

Context: Theoretical models of early accretion during the formation process of massive stars have predicted that HII regions exhibit radio variability on timescales of decades. How…

astro-ph.GA2024

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde V. The massive filament DR21

X. Zhao, X. D. Tang, C. Henkel +18

The kinetic temperature structure of the massive filament DR21 has been mapped using the IRAM 30 m telescope. This mapping employed the para-H2​CO triplet (JKa​Kc​​ = 3$_…

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