activity
19992023
most citedEpisodic formation of cometary material in the outburst of a solar-like young star

175 citations · 512 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2023

The disk of the eruptive protostar V900 Mon; a MATISSE/VLTI and MUSE/VLT perspective

F. Lykou, P. Ábrahám, F. Cruz-Sáenz de Miera +8

In this work, we study the silicate dust content in the disk of one of the youngest eruptive stars, V900 Mon, at the highest angular resolution probing down to the inner 10 au of s…

astro-ph.SR2012★ 96 cited

Star formation and disk properties in Pismis 24

M. Fang, R. van Boekel, R. R. King +6

(abridged) We investigate the properties of young stars and their disks in the NGC 6357 complex, concentrating on the most massive star cluster within the complex: Pismis 24. We di…

astro-ph.SR2011★ 95 cited

Silicate features in Galactic and extragalactic post-AGB discs

C. Gielen, J. Bouwman, H. Van Winckel +7

Aims. In this paper we study the Spitzer and TIMMI2 infrared spectra of post-AGB disc sources, both in the Galaxy and the LMC. Using the observed infrared spectra we determine the…

astro-ph.SR2011★ 31 cited

Multi-wavelength observations of the young binary system Haro 6-10: The case of misaligned discs

V. Roccatagliata, Th. Ratzka, Th. Henning +3

Context. We present a multi-wavelength, high-resolution observational survey of the young binary system Haro 6-10 (GV Tau, IRAS 04263+2426), which is harbouring one of the few know…

astro-ph.SR2011★ 48 cited

Low abundance, strong features: Window-dressing crystalline forsterite in the disk wall of HD 100546

G. D. Mulders, L. B. F. M. Waters, C. Dominik +10

Forsterite is one of the crystalline dust species that is often observed in protoplanetary disks and solar system comets. Being absent in the interstellar medium, it must be produc…

astro-ph.SR2009★ 49 cited

On the interplay between flaring and shadowing in disks around Herbig Ae/Be stars

B. Acke, M. Min, M. van den Ancker +4

Based on the SED, Herbig stars have been categorized into two observational groups, reflecting their overall disk structure: group I members have disks with a higher degree of flar…