activity
20152026
most citedWeak Turbulence in the HD 163296 Protoplanetary Disk Revealed by ALMA CO Observations

296 citations · 1k across the 7 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2026

Peering into the Midplane of the DM Tau Disk using N2H+ and DCO+

Amina Diop, Kevin Flaherty, Chunhua Qi +7

Planets form in the midplanes of protoplanetary disks, thus investigating the properties of the midplane region can shed light on the physical and chemical processes governing the…

astro-ph.SR2026

Mapping Molecular Ion Distributions in a Diverse Sample of Protoplanetary Disks

Deryl E. Long, L. Ilsedore Cleeves, Charles J. Law +10

Observations of ionization-tracing molecules in protoplanetary disks suggest that their ionization environments are diverse due to varying degrees of cosmic ray modulation, stellar…

astro-ph.EP2026

Turbulence Can Persist in the Inner Regions of Weakly-Ionized Planet Forming Disks

David G. Rea, Jacob B. Simon

Identifying the mechanisms responsible for angular momentum transport in protoplanetary disks, and the extent to which those mechanisms produce turbulence, is a crucial problem in…

astro-ph.EP2025★ 1 cited

On Linking Planet Formation Models, Protoplanetary Disk Properties, and Mature Gas Giant Exoplanet Atmospheres

Adina D. Feinstein, Richard A. Booth, Jennifer B. Bergner +34

Measuring a single elemental ratio (e.g., carbon-to-oxygen) provides insufficient information for understanding the formation mechanisms and evolution that affect our observations…

astro-ph.SR2024

Exploring the Complex Ionization Environment of the Turbulent DM Tau Disk

Deryl E. Long, L. Ilsedore Cleeves, Fred C. Adams +9

Ionization drives important chemical and dynamical processes within protoplanetary disks, including the formation of organics and water in the cold midplane and the transportation…

astro-ph.EP2024

Evidence for Non-zero Turbulence in the Protoplanetary disc around IM Lup

Kevin Flaherty, A. Meredith Hughes, Jacob B. Simon +6

The amount of turbulence in protoplanetary discs around young stars is critical for determining the efficiency, timeline, and outcomes of planet formation. It is also difficult to…