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20202026
most citedDust Populations in the Iconic Vega Planetary System Resolved by ALMA

28 citations · 55 across the 30 of their papers we have counts for

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astro-ph.EP2026

JWST/MIRI Imaging Search for Kinematically Detected Protoplanetary Candidates

G. Cugno, M. Benisty, R. Teague +32

Kinematic perturbations observed with ALMA in CO line emission provide evidence for a population of embedded giant protoplanets shaping the structure of protoplanetary disks. We pr…

astro-ph.EP2026

Empirical Constraints on the CO Snowline Transition in HD 163296: The Local CO Column and CO Optical Depth

Chunhua Qi, Takahiro Ueda, David J. Wilner +1

CO isotopologue emission is widely used to infer gas masses and volatile carbon abundances in protoplanetary disks, but converting line emission into a CO column depends on optical…

astro-ph.EP2026

An analysis of the Herbig star population and their protoplanetary disks within 1 kpc

L. M. Stapper, M. Vioque, A. J. Winter +6

Herbig stars are intermediate mass pre-main sequence stars of 1.5 to ~M and are in between low and high-mass star formation. This work provides a catalog of all 243…

astro-ph.EP2026

SMA Observations Reveal Abundant HNC Chemistry in Transition Disks

Kyle Gresko, Charles J. Law, Deryl E. Long +8

The physical and chemical conditions of protoplanetary disks shape the properties of nascent planetary systems. The line ratios and relative abundances of the HCN-HNC isomer pair a…

astro-ph.EP2026

Demographics of planet-forming disks with the SKAO

Antonio Garufi, Sebastián Pérez, John D. Ilee +21

Understanding how solid material in planet-forming disks evolves from micron-sized dust to planetary cores is a central challenge in modern astrophysics. This study has advanced dr…

astro-ph.EP2026

Substructures in Planet-Forming Disks with the SKAO

Yinhao Wu, Jessica Speedie, Sebastián Pérez +33

Disks of gas and dust orbiting young stars are the arenas and material reservoirs for planet formation. Over the past decade, multiwavelength observations, from infrared to radio,…