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Ji-Ming Shi

4 papers here

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

author position
  • first author1
  • middle author1
  • last author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP3
  • astro-ph.HE1
ORCID 0000-0002-0368-2209
same name
  • Ji-Ming Shi — 5 papers, h 13

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

most citedHydrodynamics of Embedded Planets' First Atmospheres. II. A Rapid Recycling of Atmospheric Gas

206 citations · 361 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2016★ 22 cited

How bright are the gaps in circumbinary disk systems?

Ji-Ming Shi, Julian H. Krolik

When a circumbinary disk surrounds a binary whose secondary's mass is at least ∼10−2× the primary's mass, a nearly empty cavity with radius a few times the binary sep…

astro-ph.EP2014★ 206 cited

Hydrodynamics of Embedded Planets' First Atmospheres. II. A Rapid Recycling of Atmospheric Gas

Chris W. Ormel, Ji-Ming Shi, Rolf Kuiper

Following Paper I we investigate the properties of atmospheres that form around small protoplanets embedded in a protoplanetary disc by conducting hydrodynamical simulations. These…

astro-ph.EP2014★ 86 cited

Hydrodynamics of Embedded Planets' First Atmospheres. I. A Centrifugal Growth Barrier for 2D Flows

Chris W. Ormel, Rolf Kuiper, Ji-Ming Shi

In the core accretion paradigm of planet formation, gas giants only form a massive atmosphere after their progenitors exceeded a threshold mass: the critical core mass. Most (exo)p…

astro-ph.EP2014★ 47 cited

Gravito-Turbulent Disks in 3D: Turbulent Velocities vs. Depth

Ji-Ming Shi, Eugene Chiang

Characterizing turbulence in protoplanetary disks is crucial for understanding how they accrete and spawn planets. Recent measurements of spectral line broadening promise to diagno…

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