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

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Showing astro-ph.SRShow all

12 papers · 1 filter

astro-ph.SR202114 cited

The inner circumstellar dust of the red supergiant Antares as seen with VLT/SPHERE/ZIMPOL

E. Cannon, M. Montarges, A. de Koter +6

The processes by which red supergiants lose mass are not fully understood thus-far and their mass-loss rates lack theoretical constraints. The ambient surroundings of the nearby M0…

astro-ph.SR20203 cited

VLTI images of circumbinary disks around evolved stars

Jacques Kluska, Rik Claes, Akke Corporaal +13

The new generation of VLTI instruments (GRAVITY, MATISSE) aims to produce routinely interferometric images to uncover the morphological complexity of different objects at high angu…

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.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…

astro-ph.SR2018

Modelling mid-infrared molecular emission lines from T Tauri stars

P. Woitke, M. Min, W. -F. Thi +5

We introduce a new modelling framework called FLiTs to simulate infrared line emission spectra from protoplanetary discs. This paper focuses on the mid-IR spectral region between 9…

astro-ph.SR2018

The perturbed sublimation rim of the dust disk around the post-AGB binary IRAS08544-4431

J. Kluska, M. Hillen, H. Van Winckel +4

Context: Post-Asymptotic Giant Branch (AGB) binaries are surrounded by stable dusty and gaseous disks similar to the ones around young stellar objects. Whereas significant effort i…