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Xinwu Cao

85 papers hereh-index 262k citations118 works total

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

author position
  • sole author18
  • first author21
  • middle author19
  • last author27

Across the 85 of 85 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE45
  • astro-ph30
  • astro-ph.GA9
  • astro-ph.CO1
same name
  • Xinwu Cao — 9 papers, h 2
  • Xinwu Cao — 4 papers, h 1
  • Xinwu Cao — 3 papers, h 4
  • Xinwu Cao — 3 papers
  • Xinwu Cao — 3 papers, h 1
  • Xinwu Cao — 2 papers, h 1

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
19972023
most citedThe anti-correlation between the hard X-ray photon index and the Eddington ratio in LLAGNs

141 citations · 2.6k across the 85 of their papers we have counts for

collaborators
Showing 2004Show all

4 papers · 1 filter

astro-ph2004★ 23 cited

Origin of Radio Emission from Nearby Low-Luminosity Active Galactic Nuclei

Qingwen Wu, Xinwu Cao

We use the observational data in radio, optical and X-ray wavebands, for a sample of active galactic nuclei (AGNs) with measured black hole masses, to explore the origin of radio e…

astro-ph2004★ 23 cited

On the dust tori in Palomar-Green quasars

Xinwu Cao

The dust clouds in the torus of the quasar are irradiated by the central source, and the clouds at the inner radius of the torus re-radiate mostly in the near-infrared (NIR) waveba…

astro-ph2004★ 21 cited

Are the jets accelerated from the disk coronas in some active galactic nuclei?

Xinwu Cao

We use a sample of radio-loud active galactic nuclei (AGNs) with estimated central black hole masses to explore their jet formation mechanisms. The jet power of AGNs is estimated f…

astro-ph2004★ 6 cited

Evidence for anisotropic motion of the clouds in broad-line regions of BL Lacertae objects

Xinwu Cao

The masses of central massive black holes in BL Lac objects are estimated from their host galaxy absolute magnitude at R-band by using the empirical relation between absolute magni…

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