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researcher

C. Cao

13 papers hereh-index 9460 citations30 works total

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

author position
  • first author2
  • middle author9
  • last author1

Across the 12 of 13 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA6
  • astro-ph4
  • astro-ph.CO1
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • C. Cao — 63 papers, h 28
  • C. Cao — 26 papers, h 27
  • C. Cao — 22 papers, h 10
  • C. Cao — 21 papers, h 20
  • C. Cao — 21 papers, h 9
  • C. Cao — 11 papers, h 21

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
20052019
most citedDiscovery of the broad-lined Type Ic SN 2013cq associated with the very energetic GRB 130427A

134 citations · 456 across the 13 of their papers we have counts for

collaborators
Showing 2014 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2014★ 67 cited

ALMA Observations of Warm Dense Gas in NGC 1614 --- Breaking of Star Formation Law in the Central kpc

C. K. Xu, C. Cao, N. Lu +20

We present ALMA Cycle-0 observations of the CO (6-5) line emission and of the 435um dust continuum emission in the central kpc of NGC 1614, a local luminous infrared galaxy (LIRG)…

astro-ph.GA2014★ 28 cited

Star Formation Properties in Barred Galaxies(SFB). III. Statistical Study of Bar-driven Secular Evolution using a sample of nearby barred spirals

Zhi-Min Zhou, Chen Cao, Hong Wu

Stellar bars are important internal drivers of secular evolution in disk galaxies. Using a sample of nearby spiral galaxies with weak and strong bars, we explore the relationships…

astro-ph.GA2014★ 41 cited

ALMA Observations of Warm Molecular Gas and Cold Dust in NGC 34

C. K. Xu, C. Cao, N. Lu +17

We present ALMA Cycle-0 observations of the CO (6-5) line emission (rest-frame frequency = 691.473 GHz) and of the 435μm dust continuum emission in the nuclear region of NGC 34,…

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