activity
20122026
most citedMass inventory of the giant-planet formation zone in a solar nebula analog

146 citations · 788 across the 23 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

22 papers · 1 filter

astro-ph.EP2026

The ALMA View of the Edge-on Gomez's Hamburger System: A Highly-Dynamic, Asymmetric Protoplanetary Disk Reveals the Earliest Phases of Giant Planet Formation

Charles J. Law, Jensen Lawrence, Richard Teague +18

Chemical tracers provide some of the strongest observational signatures of ongoing planet formation and localized dynamical perturbations in protoplanetary disks. In particular, su…

astro-ph.EP20251 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.EP202446 cited

JWST/NIRSpec Reveals the Nested Morphology of Disk Winds from Young Stars

Ilaria Pascucci, Tracy L. Beck, Sylvie Cabrit +15

Radially extended disk winds could be the key to unlocking how protoplanetary disks accrete and how planets form and migrate. A distinctive characteristic is their nested morpholog…

astro-ph.EP2024

Hints of planet formation signatures in a large-cavity disk studied in the AGE-PRO ALMA Large Program

Anibal Sierra, Laura M. Pérez, Carolina Agurto-Gangas +19

Detecting planet signatures in protoplanetary disks is fundamental to understanding how and where planets form. In this work, we report dust and gas observational hints of planet f…

astro-ph.EP2024

The Carbon Isotopic Ratio and Planet Formation

Edwin A. Bergin, Arthur Bosman, Richard Teague +6

We present the first detection of 13CCH in a protoplanetary disk (TW Hya). Using observations of C2H we measure CCH/13CCH = 65 +/- 20 in gas with a CO isotopic ratio of 12CO/13CO =…

astro-ph.EP2024

Molecular Gas Tracers in Young and Old Protoplanetary Disks

Dana E. Anderson, L. Ilsedore Cleeves, Geoffrey A. Blake +6

Molecular emission is used to investigate both the physical and chemical properties of protoplanetary disks. Therefore, to accurately derive disk properties, we need a thorough und…