Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar disk that is responsible for the observed infrared (IR) excess and emission lines. The influence of binarity on these phenomena remains controversial. We followed the evolution of the environment surrounding the binary Be star $\delta$ Scorpii one year before...
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January 9, 2013 (v1)Journal articleUploaded on: December 4, 2022
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September 23, 2009 (v1)Journal article
Most Wolf-Rayet stars (WR) of WC9 sub-type exhibit a dusty circumstellar envelope, but it is still a matter of debate how dust can form in their harsh environment. In a few cases, a pinwheel-like structure of the dusty envelope has been detected. Therefore, it has been suggested that dust formation in all dusty WR stars might be linked to...
Uploaded on: December 4, 2022 -
July 30, 2010 (v1)Publication
Due to the recent dramatic technological advances, infrared interferometry can now be applied to new classes of objects, resulting in exciting new science prospects, for instance, in the area of high-mass star formation. Although extensively studied at various wavelengths, the process through which massive stars form is still only poorly...
Uploaded on: December 3, 2022 -
July 28, 2010 (v1)Publication
Circumstellar disks are an essential ingredient of the formation of low-mass stars. It is unclear, however, whether the accretion-disk paradigm can also account for the formation of stars more massive than about 10 solar masses, in which strong radiation pressure might halt mass infall. Massive stars may form by stellar merging, although more...
Uploaded on: December 3, 2022 -
December 14, 2020 (v1)Conference paper
International audience
Uploaded on: February 22, 2023 -
December 14, 2020 (v1)Conference paper
International audience
Uploaded on: December 4, 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 -
July 2012 (v1)Conference paper
We present the results of the fifth Interferometric Imaging Beauty Contest. The contest consists in blind imaging of test data sets derived from model sources and distributed in the OIFITS format. Two scenarios of imaging with CHARA/MIRC-6T were offered for reconstruction: imaging a T Tauri disc and imaging a spotted red supergiant. There were...
Uploaded on: December 2, 2022 -
December 14, 2020 (v1)Conference paper
International audience
Uploaded on: December 3, 2022