activity
20062022
most citedConsistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs

379 citations · 1.5k across the 19 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2022★ 10 cited

Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Scattered light detection of a possible disk wind in RY Tau

P. -G. Valegård, C. Ginski, C. Dominik +14

Disk winds are an important mechanism for accretion and disk evolution around young stars. The accreting intermediate-mass T-Tauri star RY Tau has an active jet and a previously kn…

astro-ph.EP2022★ 39 cited

H2S and SO2 detectability in Hot Jupiters: Sulfur species as indicator of metallicity and C/O ratio

J. Polman, L. B. F. M. Waters, M. Min +2

The high cosmic abundance and the intermediate volatility and chemical properties of sulfur allow the use of sulfur-bearing species as a tracer of the chemical processes in the atm…

astro-ph.EP2020★ 42 cited

Mineral cloud and hydrocarbon haze particles in the atmosphere of the hot Jupiter JWST target WASP-43b

Ch. Helling, Y. Kawashima, V. Graham +5

Having a short orbital period and being tidally locked makes WASP-43b an ideal candidate for JWST observations. Phase curve observations of an entire orbit will enable the mapping…

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.EP2018★ 93 cited

Consistent dust and gas models for protoplanetary disks III. Models for selected objects from the FP7 DIANA project

P. Woitke, I. Kamp, S. Antonellini +17

The European FP7 project DIANA has performed a coherent analysis of a large set of observations from protoplanetary disks by means of thermo-chemical disk models. The collected dat…

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…