379 citations · 5.3k across the 87 of their papers we have counts for
7 papers · 1 filter
ALMA and NACO observations towards the young exoring transit system J1407 (V1400 Cen)
M. A. Kenworthy, P. D. Klaassen, M. Min +8
Our aim was to directly detect the thermal emission of the putative exoring system responsible for the complex deep transits observed in the light curve for the young Sco-Cen star…
Dust evolution in pre-stellar cores
Charlène Lefèvre, Laurent Pagani, Bilal Ladjelate +3
Dust grains are the building {blocks} of future planets. They evolve in size, shape and composition during the life cycle of the interstellar medium. We seek to understand the proc…
VLTI/PIONIER survey of disks around post-AGB binaries. Dust sublimation physics rules!
J. Kluska, H. Van Winckel, M. Hillen +4
Post-AGB binaries are surrounded by circumbinary disks of gas and dust that are similar to protoplanetary disks found around young stars. We aim to understand the structure of thes…
ESA Voyage 2050 White Paper: Detecting life outside our solar system with a large high-contrast-imaging mission
Ignas Snellen, Simon Albrecht, Guillem Anglada-Escude +64
In this white paper, we recommend the European Space Agency plays a proactive role in developing a global collaborative effort to construct a large high-contrast imaging space tele…
Optical polarized phase function of the HR\,4796A dust ring
J. Milli, N. Engler, H. M. Schmid +24
The scattering properties of the dust originating from debris discs are still poorly known. The analysis of scattered light is however a powerful remote-sensing tool to understand…
Consistent dust and gas models for protoplanetary disks IV. A panchromatic view of protoplanetary disks
O. Dionatos, P. Woitke, M. Guedel +17
Consistent modeling of protoplanetary disks requires the simultaneous solution of both continuum and line radiative transfer, heating/cooling balance between dust and gas and, of c…
The ARCiS framework for Exoplanet Atmospheres: The Cloud Transport Model
Chris W. Ormel, Michiel Min
Understanding of clouds is instrumental in interpreting current and future spectroscopic observations of exoplanets. Modelling clouds consistently is complex, since it involves man…