activity
20102020
most citedThe WISE View of RV Tauri Stars

83 citations · 748 across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.SR2020★ 9 cited

Rapid grain growth in post-AGB disc systems from far-infrared and sub-millimetre photometry

P. Scicluna, F. Kemper, A. Trejo +3

The timescales on which astronomical dust grows remain poorly understood, with important consequences for our understanding of processes like circumstellar disk evolution and plane…

astro-ph.SR2020★ 23 cited

Optical/near-infrared observations of the Fried Egg Nebula: Multiple shell ejections on a 100 yr timescale from a massive yellow hypergiant

E. Koumpia, R. D. Oudmaijer, V. Graham +15

Context. The fate of a massive star during the latest stages of its evolution is highly dependent on its mass-loss rate/geometry and therefore knowing the geometry of the circumste…

astro-ph.SR2019★ 33 cited

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.SR2019★ 16 cited

Resolved imaging of the AR Puppis circumbinary disk

S. Ertel, D. Kamath, M. Hillen +14

Circumbinary disks are common around post-asymptotic giant branch (post-AGB) stars with a stellar companion on orbital time scales of a few 100 to few 1000 days. The presence of a…

astro-ph.SR2018★ 36 cited

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…

astro-ph.SR2018★ 50 cited

High-resolution observations of IRAS 08544-4431. Detection of a disk orbiting a post-AGB star and of a slow disk wind

V. Bujarrabal, A. Castro-Carrizo, H. Van Winckel +4

We are studying a class of binary post-AGB stars that seem to be systematically surrounded by equatorial disks and slow outflows. Although the rotating dynamics had only been well…