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researcher

Yan-Fei Jiang

38 papers hereh-index 191.8k citations48 works total

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

author position
  • sole author1
  • first author12
  • middle author14
  • last author11

Across the 38 of 38 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE13
  • astro-ph.GA9
  • astro-ph.IM6
  • astro-ph3
  • astro-ph.CO3
  • astro-ph.EP3
same name
  • Yan-Fei Jiang — 26 papers, h 6
  • Yan-Fei Jiang — 12 papers, h 4
  • Yan-Fei Jiang — 9 papers, h 3
  • Yan-Fei Jiang — 8 papers, h 2
  • Yan-Fei Jiang — 7 papers, h 3
  • Yan-Fei Jiang — 6 papers, h 3

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
20082023
most citedA Global Three Dimensional Radiation Magneto-hydrodynamic Simulation of Super-Eddington Accretion Disks

440 citations · 2.5k across the 38 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

3 papers · 1 filter

astro-ph.EP2021★ 29 cited

Global 3D Radiation Hydrodynamic Simulations of Proto-Jupiter's Convective Envelope

Zhaohuan Zhu, Yan-Fei Jiang, Hans Baehr +3

The core accretion model of giant planet formation has been challenged by the discovery of recycling flows between the planetary envelope and the disc that can slow or stall envelo…

astro-ph.EP2019★ 59 cited

Global 3-D Radiation Magnetohydrodynamic Simulations for FU Ori's Accretion Disk and Observational Signatures of Magnetic Fields

Zhaohuan Zhu, Yan-Fei Jiang, James M. Stone

FU Ori is the prototype of FU Orionis systems which are outbursting protoplanetary disks. Magnetic fields in FU Ori's accretion disks have previously been detected using spectropol…

astro-ph.EP2019★ 205 cited

One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering

Zhaohuan Zhu, Shangjia Zhang, Yan-Fei Jiang +10

ALMA surveys have suggested that the dust in Class II disks may not be enough to explain the averaged solid mass in exoplanets, under the assumption that the mm disk continuum emis…

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