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Min-Kai Lin

47 papers hereh-index 17960 citations51 works total

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

author position
  • sole author11
  • first author12
  • middle author6
  • last author18

Across the 47 of 47 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP45
  • astro-ph.GA1
  • astro-ph.SR1
same name
  • Min-Kai Lin — 10 papers, h 3
  • Min-Kai Lin — 6 papers, h 2
  • Min-Kai Lin — 2 papers, h 0

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
20102024
most citedCooling Requirements for the Vertical Shear Instability in Protoplanetary Disks

169 citations · 1.4k across the 47 of their papers we have counts for

collaborators
Showing 2020Show all

4 papers · 1 filter

astro-ph.EP2020★ 33 cited

Stratified and vertically-shearing streaming instabilities in protoplanetary disks

Min-Kai Lin

Under the right conditions, the streaming instability between imperfectly coupled dust and gas is a powerful mechanism for planetesimal formation as it can concentrate dust grains…

astro-ph.EP2020★ 12 cited

A Machine Learning model to infer planet masses from gaps observed in protoplanetary disks

Sayantan Auddy, Min-Kai Lin

Observations of bright protoplanetary disks often show annular gaps in their dust emission. One interpretation of these gaps is disk-planet interaction. If so, fitting models of pl…

astro-ph.EP2020★ 17 cited

Migrating Low-Mass Planets in Inviscid Dusty Protoplanetary Discs

He-Feng Hsieh, Min-Kai Lin

Disc-driven planet migration is integral to the formation of planetary systems. In standard, gas-dominated protoplanetary discs, low-mass planets or planetary cores undergo rapid i…

astro-ph.EP2020★ 78 cited

How efficient is the streaming instability in viscous protoplanetary disks?

Kan Chen, Min-Kai Lin

The streaming instability is a popular candidate for planetesimal formation by concentrating dust particles to trigger gravitational collapse. However, its robustness against physi…

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