activity
20052026
most citedMapping the radial structure of AGN tori

156 citations · 3k across the 144 of their papers we have counts for

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Showing 2010Show all

7 papers · 1 filter

astro-ph.SR2010★ 90 cited

Imaging the spinning gas and dust in the disc around the supergiant A[e] star HD62623

Florentin Millour, Anthony Meilland, Olivier Chesneau +5

Context. To progress in the understanding of evolution of massive stars one needs to constrain the mass-loss and determine the phenomenon responsible for the ejection of matter an…

astro-ph.SR2010

Imaging "Pinwheel"nebulae with optical long-baseline interferometry

Florentin Millour, Thomas Driebe, José Groh +4

Dusty Wolf-Rayet stars are few but remarkable in terms of dust production rates (up to one millionth of solar mass per year). Infrared excesses associated to mass-loss are found in…

astro-ph.SR2010

Images of unclassified and supergiant B[e] stars disks with interferometry

Florentin Millour, Anthony Meilland, Olivier Chesneau +5

B[e] stars are among the most peculiar objects in the sky. This spectral type, characterised by allowed and forbidden emission lines, and a large infrared excess, does not represen…

astro-ph.SR2010★ 10 cited

An investigation of the close environment of beta Cep with the VEGA/CHARA interferometer

N. Nardetto, D. Mourard, I. Tallon-Bosc +22

High-precision interferometric measurements of pulsating stars help to characterize their close environment. In 1974, a close companion was discovered around the pulsating star bet…

astro-ph.IM2010★ 4 cited

The third version of the AMBER data reduction software

Fabien Malbet, Gilles Duvert, Florentin Millour +7

We present the third release of the AMBER data reduction software by the JMMC. This software is based on core algorithms optimized after several years of operation. An optional gra…

astro-ph.SR2010★ 27 cited

Time, spatial, and spectral resolution of the Halpha line-formation region of Deneb and Rigel with the VEGA/CHARA interferometer

Olivier Chesneau, Luc Dessart, D. Mourard +22

BA-type supergiants are amongst the most optically-bright stars. They are observable in extragalactic environments, hence potential accurate distance indicators. Emission activity…