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Chen Hu

57 papers hereh-index 313k citations91 works total

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

author position
  • first author6
  • middle author42
  • last author5

Across the 53 of 57 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA33
  • astro-ph.CO10
  • astro-ph.HE7
  • astro-ph6
  • astro-ph.IM1
same name
  • Chen Hu — 33 papers, h 12
  • Chen Hu — 16 papers, h 7
  • Chen Hu — 7 papers, h 3
  • Chen Hu — 5 papers, h 6
  • Chen Hu — 4 papers, h 5
  • Chen Hu — 4 papers, h 11

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
20052025
most citedSupermassive black holes with high accretion rates in active galactic nuclei: I. First results from a new reverberation mapping campaign

238 citations · 3.4k across the 57 of their papers we have counts for

collaborators
Showing 2009Show all

3 papers · 1 filter

astro-ph.CO2009★ 92 cited

Implications of infalling Fe II - emitting clouds in active galactic nuclei: anisotropic properties

Gary J. Ferland, Chen Hu, Jian-Min Wang +4

We investigate consequences of the discovery that Fe II emission in quasars, one of the spectroscopic signatures of "Eigenvector 1", may originate in infalling clouds. Eigenvector…

astro-ph.CO2009★ 15 cited

Evolution of gaseous disk viscosity driven by supernova explosion in star-forming galaxies at high redshift

Jian-Min Wang, Chang-Shuo Yan, Yan-Rong Li +5

Motivated by Genzel et al.'s observations of high-redshift star-forming galaxies, containing clumpy and turbulent rings or disks, we build a set of equations describing the dynamic…

astro-ph.GA2009★ 66 cited

Episodic Random Accretion and the Cosmological Evolution of Supermassive Black Hole Spins

J. -M. Wang, C. Hu, Y. -R. Li +7

The growth of supermassive black holes (BHs) located at the centers of their host galaxies comes mainly from accretion of gas, but how to fuel them remains an outstanding unsolved…

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