International audience
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November 17, 2021 (v1)Journal articleUploaded on: February 22, 2023
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November 17, 2021 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
2018 (v1)Journal article
During the last two decades, the first generation of beam combiners at the Very Large Telescope Interferometer has proved the importance of optical interferometry for high-angular resolution astrophysical studies in the near- and mid-infrared. With the advent of 4-beam combiners at the VLTI, the u - v coverage per pointing increases...
Uploaded on: December 3, 2022 -
2020 (v1)Journal article
Context. Shadows in scattered light images of protoplanetary disks are a common feature and support the presence of warps or misalignments between disk regions. These warps are possibly caused by an inclined (sub-)stellar companion embedded in the disk.Aims. We aim to study the morphology of the protoplanetary disk around the Herbig Ae star HD...
Uploaded on: December 4, 2022 -
December 2021 (v1)Journal article
Very Large Telescope Inerferometer (VLTI) schools have nearly a 20-year history and have trained a significant fraction of today's optical interferometrists who use high-angular-resolution techniques on a regular basis. Very early in the development of the VLTI, training was identified by the community as a necessary tool, as the expertise in...
Uploaded on: December 4, 2022 -
June 2016 (v1)Conference paper
We present an overview of the scientific potential of MATISSE, the Multi Aperture mid-Infrared SpectroScopic Experiment for the Very Large Telescope Interferometer. For this purpose we outline selected case studies from various areas, such as star and planet formation, active galactic nuclei, evolved stars, extrasolar planets, and solar system...
Uploaded on: December 3, 2022 -
July 17, 2022 (v1)Conference paper
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Uploaded on: December 4, 2022 -
September 27, 2023 (v1)Journal article
Abstract From Nov. 2019 to May 2020, the red supergiant star Betelgeuse experienced an unprecedented drop of brightness in the visible domain called the great dimming event. Large atmospheric dust clouds and large photospheric convective features are suspected to be responsible for it. To better understand the dimming event, we used...
Uploaded on: October 14, 2023 -
June 10, 2018 (v1)Conference paper
International audience
Uploaded on: December 4, 2022