most citedVLTI monitoring of the dust formation event of the Nova V1280 Sco

40 citations · 73 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph200812 cited

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…

astro-ph200821 cited

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…

astro-ph200840 cited

VLTI monitoring of the dust formation event of the Nova V1280 Sco

Olivier Chesneau, Dipankar Banerjee, F. Millour +13

We present the first high spatial resolution monitoring of the dust forming nova V1280 Sco performed with the Very Large Telescope Interferometer (VLTI). Spectra and visibilities w…

astro-ph200738 cited

A disc in the heart of the Ant nebula

Foteini Lykou, Olivier Chesneau, Eric Lagadec +1

We present the discovery of a silicate disc at the centre of the planetary nebula Mz3 (the Ant). The nebula was observed with MIDI on the Very Large Telescope Interferometer (VLTI)…

astro-ph200738 cited

A silicate disk in the heart of the Ant

Olivier Chesneau, Foteini Lykou, Bruce Balick +6

We aim at getting high spatial resolution information on the dusty core of bipolar planetary nebulae to directly constrain the shaping process. Methods: We present observations of…

astro-ph200649 cited

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…