most citedExploring dust around HD142527 down to 0.025" / 4au using SPHERE/ZIMPOL

100 citations · 252 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.SR201724 cited

The protoplanetary system HD 100546 in H polarized light from SPHERE/ZIMPOL. A bar-like structure across the disk gap?

I. Mendigutía, R. D. Oudmaijer, A. Garufi +7

HD 100546 is one of the few known pre-main-sequence stars that may host a planetary system in its disk. We analyze new VLT/SPHERE/ZIMPOL polarimetric images of HD 100546 with filte…

astro-ph.EP201718 cited

Three years of SPHERE: the latest view of the morphology and evolution of protoplanetary discs

Antonio Garufi, Myriam Benisty, Tomas Stolker +11

Spatially resolving the immediate surroundings of young stars is a key challenge for the planet formation community. SPHERE on the VLT represents an important step forward by incre…

astro-ph.EP201769 cited

Variable dynamics in the inner disk of HD 135344B revealed with multi-epoch scattered light imaging

Tomas Stolker, Mike Sitko, Bernard Lazareff +12

We present multi-epoch VLT/SPHERE observations of the protoplanetary disk around HD 135344B (SAO 206462). The -band scattered light imagery reveal, with high spatial resolution…

astro-ph.EP2017100 cited

Exploring dust around HD142527 down to 0.025" / 4au using SPHERE/ZIMPOL

H. Avenhaus, S. P. Quanz, H. M. Schmid +25

We have observed the protoplanetary disk of the well-known young Herbig star HD 142527 using ZIMPOL Polarimetric Differential Imaging with the VBB (Very Broad Band, ~600-900nm) fil…

astro-ph.EP201741 cited

New constraints on the disk characteristics and companion candidates around T Cha with VLT/SPHERE

A. Pohl, E. Sissa, M. Langlois +34

The transition disk around the T Tauri star T Cha possesses a large gap, making it a prime target for high-resolution imaging in the context of planet formation. We aim to find sig…

astro-ph.EP2016

Discovery of concentric broken rings at sub-arcsec separations in the HD 141569A gas-rich, debris disk with VLT/SPHERE

C. Perrot, A. Boccaletti, E. Pantin +45

Transition disks correspond to a short stage between the young protoplanetary phase and older debris phase. Along this evolutionary sequence, the gas component disappears leaving r…