activity
20062023
most citedA close look into the carbon disk at the core of the planetary nebula CPD-568032

37 citations · 118 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2023★ 10 cited

The dusty circumstellar environment of Betelgeuse during the Great Dimming as seen by VLTI/MATISSE

E. Cannon, M. Montargès, A. de Koter +23

The 'Great Dimming' of the prototypical red supergiant Betelgeuse, which occurred between December 2019 and April 2020, gives us unprecedented insight into the processes occurring…

astro-ph.SR2022★ 5 cited

Locating dust and molecules in the inner circumstellar environment of R~Sculptoris with MATISSE

Julien Drevon, Florentin Millour, Pierre Cruzalèbes +49

AGB stars are one of the main sources of dust production in the Galaxy. However, it is not clear what this process looks like and where the dust is condensing in the circumstellar…

astro-ph.SR2022★ 18 cited

The disk of FU Orionis viewed with MATISSE/VLTI: first interferometric observations in and bands

F. Lykou, P. Ábrahám, L. Chen +30

The disk of FU Orionis is marginally resolved with MATISSE, suggesting that the region emitting in the thermal infrared is rather compact. An upper limit of mas (in…

astro-ph.IM2022★ 3 cited

Improving the diameters of interferometric calibrators with MATISSE

S. Robbe-Dubois, P. Cruzalèbes, Ph. Berio +16

A good knowledge of the angular diameters of stars used to calibrate the observables in stellar interferometry is fundamental. As the available precision for giant stars is worse t…

astro-ph.SR2021★ 12 cited

The extended atmosphere and circumstellar environment of the cool evolved star VX Sagittarii as seen by MATISSE

A. Chiavassa, K. Kravchenko, M. Montargès +50

Context. VX Sgr is a cool, evolved, and luminous red star whose stellar parameters are difficult to determine, which affects its classification. Aims. We aim to spatially resolve t…

astro-ph.IM2021★ 3 cited

MATISSE, the VLTI mid-infrared imaging spectro-interferometer

B. Lopez, S. Lagarde, R. G. Petrov +150

Context:Optical interferometry is at a key development stage. ESO's VLTI has established a stable, robust infrastructure for long-baseline interferometry for general astronomical o…