activity
20102026
most citedThe Disk Substructures at High Angular Resolution Project (DSHARP): I. Motivation, Sample, Calibration, and Overview

1.1k citations · 14.1k across the 130 of their papers we have counts for

collaborators
Showing 2021Show all

8 papers · 1 filter

astro-ph.EP2021★ 41 cited

Large gaps and high accretion rates in photoevaporative transition disks with a dead zone

Matías Gárate, Timmy N. Delage, Jochen Stadler +7

Observations of young stars hosting transition disks show that several of them have high accretion rates, despite their disks presenting extended cavities in their dust component.…

astro-ph.EP2021★ 16 cited

Mass determination of protoplanetary disks from dust evolution

Riccardo Franceschi, Tilman Birnstiel, Thomas Henning +3

The mass of protoplanetary disks is arguably one of their most important quantities shaping their evolution toward planetary systems, but it remains a challenge to determine this q…

astro-ph.EP2021★ 21 cited

The formation of wide exoKuiper belts from migrating dust traps

E. Miller, S. Marino, S. M. Stammler +4

The question of what determines the width of Kuiper belt analogues (exoKuiper belts) is an open one. If solved, this understanding would provide valuable insights into the architec…

astro-ph.EP2021★ 12 cited

Dust entrainment in photoevaporative winds: Densities and imaging

R. Franz, B. Ercolano, S. Casassus +5

X-ray- and EUV- (XEUV-) driven photoevaporative winds acting on protoplanetary disks around young T-Tauri stars may crucially impact disk evolution, affecting both gas and dust dis…

astro-ph.EP2021★ 31 cited

Thermal Wave Instability as an Origin of Gap and Ring Structures in Protoplanetary Disks

Takahiro Ueda, Mario Flock, Tilman Birnstiel

Recent millimeter and infrared observations have shown that gap and ring-like structures are common in both dust thermal emission and scattered-light of protoplanetary disks. We in…

astro-ph.EP2021★ 4 cited

First 3-D grid-based gas-dust simulations of circumstellar disks with an embedded planet

Fabian Binkert, Judit Szulágyi, Til Birnstiel

Substructures are ubiquitous in high resolution (sub-)millimeter continuum observations of circumstellar disks. They are possibly caused by forming planets embedded in the disk. To…