activity
20142026
most citedGaps, Rings, and Non-Axisymmetric Structures in Protoplanetary Disks - From Simulations to ALMA Observations

379 citations · 497 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.EP2026

Spatial distribution of water ice in the protoplanetary silhouette disk d216-0939

J. S. Martin, S. Wolf, A. Potapov +4

The composition of rocky planets depends on the dust in their natal protoplanetary disk (PPD), potentially containing water ice. Crystalline water ice was detected in the PPD d216-…

astro-ph.EP2026

Substructures Induced by Dust Drag in Protoplanetary Disks

Jiaqing Bi, Mario Flock, Dominik Ostertag +2

Dust substructures observed in protoplanetary disks are commonly attributed to embedded planets; however, intrinsic gas-dust interactions can also generate complex morphologies. We…

astro-ph.EP2025

The MATISSE view of the inner region of the RY Tau protoplanetary disk

J. S. Martin, J. Kobus, J. Varga +44

The T-Tauri type young stellar object RY Tau exhibits a dust depleted inner cavity characteristic of a transition disk. We constrain the spatial distribution and mineralogy of dust…

astro-ph.SR2025

Feasibility of interferometric observations and characterization of planet-induced structures at sub au to au scales in protoplanetary disks

Lukas Hildebrandt, Anton Krieger, Hubert Klahr +3

Interferometric observations of protoplanetary disks by VLTI and ALMA have greatly improved our understanding of the detailed structure of these planetary birthplaces. These observ…

astro-ph.EP2025★ 4 cited

Monte Carlo post-processing for radiation hydro simulations of accreting planets in protoplanetary disks

Anton Krieger, Hubert Klahr, Julio David Melon Fuksman +1

This paper is part of a series investigating the observational appearance of planets accreting from their nascent protoplanetary disk (PPD). We evaluate the differences between gas…

astro-ph.EP2024★ 9 cited

Dust mass in protoplanetary disks with porous dust opacities

Yao Liu, Hélène Roussel, Hendrik Linz +8

ALMA surveys have suggested that protoplanetary disks are not massive enough to form the known exoplanet population, under the assumption that the millimeter continuum emission is…

astro-ph.SR2024★ 10 cited

Mid-infrared evidence for iron-rich dust in the multi-ringed inner disk of HD 144432

J. Varga, L. B. F. M. Waters, M. Hogerheijde +40

Context. Rocky planets form by the concentration of solid particles in the inner few au regions of planet-forming disks. Their chemical composition reflects the materials in the di…

astro-ph.SR2023★ 7 cited

Shaping the CO snowline in protoplanetary disks

S. Gavino, J. Kobus, A. Dutrey +4

Characterizing the dust thermal structure in protoplanetary disks is a fundamental task as the dust surface temperature can affect both the planetary formation and the chemical evo…

astro-ph.EP2016★ 88 cited

Gaps, rings, and non-axisymmetric structures in protoplanetary disks - Emission from large grains

J. P. Ruge, M. Flock, S. Wolf +5

Dust grains with sizes around (sub)mm are expected to couple only weakly to the gas motion in regions beyond 10 au of circumstellar disks. In this work, we investigate the influenc…

astro-ph.EP2014★ 379 cited

Gaps, Rings, and Non-Axisymmetric Structures in Protoplanetary Disks - From Simulations to ALMA Observations

M. Flock, J. P. Ruge, N. Dzyurkevich +3

Recent observations by the Atacama Large Millimeter/submillimeter Array (ALMA) of disks around young stars revealed distinct asymmetries in the dust continuum emission. In this wor…