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Chao‐Chin Yang

3 papers here

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

author position
  • middle author2
  • last author1

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

fields
  • astro-ph.EP3
ORCID 0000-0003-2589-5034

identity via Semantic Scholar / OpenAlex

most citedProbing Conditions for Strong Clumping by the Streaming Instability: Small Dust Grains and Low Dust-to-gas Density Ratio

1 citations · 1 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.EP2025

On the Gravitational Collapse of Small Dust Grains in Self-gravitating Disk Structures

Hans Baehr, Ken Rice, Chao-Chin Yang +1

Planet formation may begin much earlier than previously expected, when the protoplanetary disk is still massive and gravitationally unstable. It has been proposed that solid grains…

astro-ph.EP2025

Bridging Unstratified and Stratified Simulations of the Streaming Instability for τs​=0.1 Grains

Jeonghoon Lim, Stanley A. Baronett, Jacob B. Simon +4

The streaming instability (SI), driven by aerodynamic coupling between solids and the gas under a global radial pressure gradient, concentrates solids and facilitates planetesimal…

astro-ph.EP2024★ 1 cited

Probing Conditions for Strong Clumping by the Streaming Instability: Small Dust Grains and Low Dust-to-gas Density Ratio

Jeonghoon Lim, Jacob B. Simon, Rixin Li +5

The streaming instability (SI) is a leading mechanism for concentrating solid particles into regions dense enough to form planetesimals. Its efficiency in clumping particles depend…

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