activity
20242026
most citedDust-Gas Coupling in Turbulence- and MHD Wind-Driven Protoplanetary Disks: Implications for Rocky Planet Formation

13 citations · 27 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2026

Formation of Water-rich Giant Planet Satellites at Decretion Disk Ice Lines

Teng Ee Yap, David J. Stevenson

The volatile budgets of giant planet satellites are critical to unraveling the origin of their building blocks within the circumplanetary disks that hosted them. The Galilean moons…

astro-ph.EP2026★ 2 cited

Callisto's Nonresonant Orbit as an Outcome of Circum-Jovian Disk Substructure

Teng Ee Yap, Konstantin Batygin

The Galilean moons of Io, Europa, and Ganymede exhibit a 4:2:1 commensurability in their mean motions, a configuration known as the Laplace resonance. The prevailing view for the o…

astro-ph.EP2025★ 9 cited

Infall and Disk Processes - the Message from Meteorites

François L. H. Tissot, Christoph Burkhardt, Aleksandra Kuznetsova +5

How do planetary systems, in general, and our own Solar System (SS), in particular, form? In conjunction, Astronomy and Isotope Cosmochemistry provide us with powerful tools to ans…

astro-ph.EP2024★ 3 cited

Early Solar System Turbulence Constrained by High Oxidation States of the Oldest Non-Carbonaceous Planetesimals

Teng Ee Yap, Konstantin Batygin, François L. H. Tissot

Early Solar System (SS) planetesimals constitute the parent bodies of most meteorites investigated today. Nucleosynthetic isotope anomalies of bulk meteorites have revealed a dicho…

astro-ph.EP2024★ 13 cited

Dust-Gas Coupling in Turbulence- and MHD Wind-Driven Protoplanetary Disks: Implications for Rocky Planet Formation

Teng Ee Yap, Konstantin Batygin

The degree of coupling between dust particles and their surrounding gas in protoplanetary disks is quantified by the dimensionless Stokes number. The Stokes number (St) governs par…