157 citations · 1.9k across the 58 of their papers we have counts for
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The environment of the fast rotating star Achernar - Thermal infrared interferometry with VLTI/MIDI and SIMECA modeling
Pierre Kervella, Armando Domiciano De Souza, Samer Kanaan +3
Context: As is the case of several other Be stars, Achernar is surrounded by an envelope, recently detected by near-IR interferometry. Aims: We search for the signature of circumst…
delta Cen: a new binary Be star detected by VLTI/AMBER spectro-interferometry
Anthony Meilland, Florentin Millour, Philippe Stee +5
We study the Be star Cen circumstellar disk using long-baseline interferometry which is the only observing technique capable of resolving spatially and spectroscopically object…
The origin of hydrogen line emission for five Herbig Ae/Be stars spatially resolved by VLTI/AMBER spectro-interferometry
S. Kraus, K. -H. Hofmann, M. Benisty +14
To trace the accretion and outflow processes around YSOs, diagnostic spectral lines such as the BrG 2.166 micron line are widely used, although due to a lack of spatial resolution,…
An asymmetry detected in the disk of Kappa CMa with the AMBER/VLTI
Anthony Meilland, Florentin Millour, Philippe Stee +7
Aims. We study the geometry and kinematics of the circumstellar environment of the Be star Kappa CMa in the Br gamma emission line and its nearby continuum. Methods. We use the VLT…
First direct detection of a Keplerian rotating disk around the Be star Arae using the VLTI/AMBER instrument
Anthony Meilland, Philippe Stee, Martin Vannier +9
Aims. We aim to study the geometry and kinematics of the disk around the Be star Arae as a function of wavelength, especially across the Br emission line. The main purpose o…
Be stars: one ring to rule them all?
Anthony Meilland, Philippe Stee, Juan Zorec +1
Aims. We report theoretical spectral energy distributions (SEDs), Br line profiles and visibilities for two scenarios that can explain the disk dissipation of active hot stars a…