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researcher

C. Hao

29 papers hereh-index 8266 citations34 works total

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

author position
  • first author6
  • middle author20
  • last author2

Across the 28 of 29 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA23
  • astro-ph.SR3
  • gr-qc2
  • astro-ph.IM1
same name
  • C. Hao — 34 papers, h 18
  • C. Hao — 9 papers, h 27
  • C. Hao — 5 papers, h 3
  • C. Hao — 3 papers, h 6
  • C. Hao — 3 papers, h 1
  • C. Hao — 3 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
20202026
most citedEvolution of the local spiral structure of the Milky Way revealed by open clusters

65 citations · 386 across the 27 of their papers we have counts for

collaborators
Showing 2023Show all

4 papers · 1 filter

astro-ph.GA2023

Kinematics of the Local Spiral Structure Revealed by Young Stars in \emph{Gaia}~DR3

Dejian Liu, Ye Xu, Chaojie Hao +4

Using young open clusters and O--B2-type stars in~\emph{Gaia}~DR3, we investigate the kinematics of the local spiral structure. In general, the young sources in the outer spiral ar…

astro-ph.GA2023★ 9 cited

Distributions and Physical Properties of Molecular Clouds in the Third Galactic Quadrant: l = [219.75, 229.75]∘ and b = [-5.25, 5.25]∘

Yiwei Dong, Yan Sun, Ye Xu +11

We present the results of an unbiased 12CO/13CO/C18O (J = 1-0) survey in a portion of the third Galactic quadrant (TGQ): l = [219.75, 229.75]∘ and b = […

astro-ph.GA2023★ 4 cited

Unveiling the initial conditions of open star cluster formation

C. J. Hao, Y. Xu, L. G. Hou +2

Open clusters (OCs) are infrequent survivors of embedded clusters gestated in molecular clouds. Up to now, little is known about the initial conditions for the formation of OCs. He…

astro-ph.GA2023★ 45 cited

What Does the Milky Way Look Like?

Y. Xu, C. J. Hao, D. J. Liu +5

In spite of much work, the overall spiral structure morphology of the Milky Way remains somewhat uncertain. In the last two decades, accurate distance measurements have provided us…

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