379 citations · 1k across the 11 of their papers we have counts for
11 papers
SimAb: A simple, fast and flexible model to assess the effects of planet formation on the atmospheric composition of gas giants
N. Khorshid, M. Min, J. M. Désert +2
We present a basic, fast, and flexible planet formation model, called SimAb (Simulating Abundances), to form giant planets and study their primary atmospheric composition soon afte…
Dusty tails of evaporating exoplanets. II. Physical modelling of the KIC 12557548b light curve
R. van Lieshout, M. Min, C. Dominik +7
Evaporating rocky exoplanets, such as KIC 12557548b, eject large amounts of dust grains, which can trail the planet in a comet-like tail. When such objects occult their host star,…
Herschel detects oxygen in the beta Pictoris debris disk
A. Brandeker, G. Cataldi, G. Olofsson +28
The young star beta Pictoris is well known for its dusty debris disk, produced through the grinding down by collisions of planetesimals, kilometre-sized bodies in orbit around the…
Consistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs
P. Woitke, M. Min, C. Pinte +19
We propose a set of standard assumptions for the modelling of Class II and III protoplanetary disks, which includes detailed continuum radiative transfer, thermo-chemical modelling…
Dusty tails of evaporating exoplanets. I. Constraints on the dust composition
R. van Lieshout, M. Min, C. Dominik
Recently, two exoplanet candidates have been discovered, KIC 12557548b and KOI-2700b, whose transit profiles show evidence for a comet-like tail of dust trailing the planet, though…
Near-infrared emission from sublimating dust in collisionally active debris disks
R. van Lieshout, C. Dominik, M. Kama +1
Hot exozodiacal dust is thought to be responsible for excess near-infrared (NIR) emission emanating from the innermost parts of some debris disks. The origin of this dust, however,…