activity
20032026
most citedDiscovery of a planetary-mass companion within the gap of the transition disk around PDS 70

700 citations · 3.9k across the 49 of their papers we have counts for

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11 papers · 1 filter

astro-ph2008★ 27 cited

A parameter study of self-consistent disk models around Herbig AeBe stars

J. Meijer, C. Dominik, A. de Koter +3

We present a parameter study of self-consistent models of protoplanetary disks around Herbig AeBe stars. We use the code developed by Dullemond and Dominik, which solves the 2D rad…

astro-ph2008★ 4 cited

10 m interferometry of disks around young stars

Roy van Boekel

This contribution reviews results from interferometric observations of circumstellar disks around young stars of 3 M, performed with the MIDI instrument operati…

astro-ph2008★ 1 cited

Dissecting Massive YSOs with Mid-Infrared Interferometry

H. Linz, Th. Henning, B. Stecklum +4

The very inner structure of massive YSOs is difficult to trace. With conventional observational methods we often identify structures still several hundreds of AU in size. But we al…

astro-ph2007★ 78 cited

Evolution of dust and ice features around FU Orionis objects

S. P. Quanz, Th. Henning, J. Bouwman +5

(abridged) We present spectroscopy data for a sample of 14 FUors and 2 TTauri stars observed with the Spitzer Space Telescope or with the Infrared Space Observatory (ISO). Based on…

astro-ph2006★ 31 cited

A compact dusty disk around the Herbig Ae star HR 5999 resolved with VLTI / MIDI

Thomas Preibisch, Stefan Kraus, Thomas Driebe +2

We have used mid-infrared long-baseline interferometry with MIDI at the VLTI to resolve the circumstellar material around the Herbig Ae star HR 5999, providing the first direct mea…

astro-ph2005★ 32 cited

Flaring and self-shadowed disks around Herbig Ae stars: simulations for 10 micron interferometers

R. van Boekel, C. P. Dullemond, C. Dominik

We present simulations of the interferometric visibilities of Herbig Ae star disks. We investigate whether interferometric measurements in the 10 micrometer atmospheric window are…