activity
20032022
most citedThe shape and composition of interstellar silicate grains

209 citations · 1.2k across the 32 of their papers we have counts for

collaborators
Showing 2019Show all

7 papers · 1 filter

astro-ph.EP20195 cited

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…

astro-ph.GA20194 cited

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…

astro-ph.SR2019

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…

astro-ph.EP2019

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…

astro-ph.EP201957 cited

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…

astro-ph.SR201932 cited

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…