activity
20052021
most citedSearchCal: a Virtual Observatory tool for searching calibrators in optical long baseline interferometry. I: The bright object case

164 citations · 554 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2021★ 12 cited

Mid-infrared circumstellar emission of the long-period Cepheid l Carinae resolved with VLTI/MATISSE

V. Hocdé, N. Nardetto, A. Matter +149

The nature of circumstellar envelopes (CSE) around Cepheids is still a matter of debate. The physical origin of their infrared (IR) excess could be either a shell of ionized gas, o…

astro-ph.SR2018★ 20 cited

Physical properties of beta Lyr A and its opaque accretion disk

D. Mourard, M. Broz, J. Nemravova +23

Mass exchange and mass loss in close binaries can significantly affect their evolution, but a complete self-consistent theory of these processes is still to be developed. Processes…

astro-ph.EP2017★ 8 cited

The peculiar fast-rotating star 51 Oph probed by VEGA/CHARA

Narges Jamialahmadi, Philippe Berio, Anthony Meilland +15

Stellar rotation is a key in our understanding of both mass-loss and evolution of intermediate and massive stars. It can lead to anisotropic mass-loss in the form of radiative wind…

astro-ph.SR2016★ 24 cited

VEGA/CHARA interferometric observations of Cepheids. I. A resolved structure around the prototype classical Cepheid delta Cep in the visible spectral range

N. Nardetto, A. Mérand, D. Mourard +23

The B-W method is used to determine the distance of Cepheids and consists in combining the angular size variations of the star, as derived from infrared surface-brightness relation…

astro-ph.IM2016★ 1 cited

An overview of the mid-infrared spectro-interferometer MATISSE: science, concept, and current status

A. Matter, B. Lopez, P. Antonelli +104

MATISSE is the second-generation mid-infrared spectrograph and imager for the Very Large Telescope Interferometer (VLTI) at Paranal. This new interferometric instrument will allow…

astro-ph.SR2015★ 78 cited

Spectral and spatial imaging of the Be+sdO binary phi Persei

D. Mourard, J. D. Monnier, A. Meilland +25

The rapidly rotating Be star phi Persei was spun up by mass and angular momentum transfer from a now stripped-down, hot subdwarf companion. Here we present the first high angular r…