activity
20182021
most citedDisk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Late infall causing disk misalignment and dynamic structures in SU Aur

110 citations · 581 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2021★ 1 cited

A SPHERE survey of self-shadowed planet-forming disks

A. Garufi, C. Dominik, C. Ginski +20

To date, nearly two hundred planet-forming disks have been imaged with high resolution. Our propensity to study bright and extended objects is however biasing our view of the disk…

astro-ph.EP2021★ 9 cited

An extended scattered light disk around AT Pyx -- Possible planet formation in a cometary globule

C. Ginski, R. Gratton, A. Bohn +35

To understand how the multitude of planetary systems that have been discovered come to be, we need to study systems at different evolutionary stages, with different central stars b…

astro-ph.EP2021★ 20 cited

Self-consistent modelling of the dust component in protoplanetary and circumplanetary disks: the case of PDS 70

B. Portilla-Revelo, I. Kamp, Ch. Rab +4

Direct observations of young stellar objects are important to test established theories of planet formation. PDS 70 is one of the few cases where robust evidence favours the presen…

astro-ph.EP2021★ 110 cited

Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Late infall causing disk misalignment and dynamic structures in SU Aur

C. Ginski, S. Facchini, J. Huang +19

Gas-rich circumstellar disks are the cradles of planet formation. As such, their evolution will strongly influence the resulting planet population. In the ESO DESTINYS large progra…

astro-ph.SR2020★ 40 cited

Interpreting high spatial resolution line observations of planet-forming disks with gaps and rings -- The case of HD 163296

Ch. Rab, I. Kamp, C. Dominik +5

Spatially resolved continuum observations of planet-forming disks show prominent ring and gap structures in their dust distribution. However, the picture from gas observations is m…

astro-ph.EP2020★ 40 cited

Spirals inside the millimeter cavity of transition disk SR 21

G. A. Muro-Arena, C. Ginski, C. Dominik +22

Hydrodynamical simulations of planet-disk interactions suggest that planets may be responsible for a number of the sub-structures frequently observed in disks in both scattered lig…

astro-ph.EP2019★ 67 cited

Shadowing and multiple rings in the protoplanetary disk of HD 139614

G. A. Muro-Arena, M. Benisty, C. Ginski +20

Shadows in scattered light images of protoplanetary disks are a common feature and support the presence of warps or misalignments between disk regions. These warps are possibly due…

astro-ph.SR2019★ 19 cited

Observing the gas component of circumplanetary disks around wide-orbit planet-mass companions in the (sub)mm regime

Ch. Rab, I. Kamp, C. Ginski +6

Several detections of wide-orbit planet-mass/sub-stellar companions around young solar-like stars were reported in the last decade. The origin of those possible planets is still un…

astro-ph.SR2019★ 66 cited

Spatial segregation of dust grains in transition disks. SPHERE observations of 2MASS J16083070-3828268 and RXJ1852.3-3700

M. Villenave, M. Benisty, W. R. F. Dent +27

Context. The mechanisms governing the opening of cavities in transition disks are not fully understood. Several processes have been proposed but their occurrence rate is still unkn…

astro-ph.SR2019★ 25 cited

Discovery of a directly imaged disk in scattered light around the Sco-Cen member Wray 15-788

A. J. Bohn, M. A. Kenworthy, C. Ginski +10

As part of our on-going survey we have carried out high-contrast imaging with VLT/SPHERE/IRDIS to obtain polarized and total intensity images of the young (Myr old)…

astro-ph.EP2018★ 107 cited

Shadows and asymmetries in the T Tauri disk HD 143006: Evidence for a misaligned inner disk

M. Benisty, A. Juhasz, S. Facchini +13

While planet formation is thought to occur early in the history of a protoplanetary disk, the presence of planets embedded in disks, or of other processes driving disk evolution, m…

astro-ph.EP2018★ 77 cited

Dust modeling of the combined ALMA and SPHERE datasets of HD163296. Is HD163296 really a Meeus group II disk?

G. A. Muro-Arena, C. Dominik, L. B. F. M. Waters +20

Context. Multi-wavelength observations are indispensable in studying disk geometry and dust evolution processes in protoplanetary disks. Aims. We aimed to construct a 3-dimensional…