activity
20052008
most citedThe origin of hydrogen line emission for five Herbig Ae/Be stars spatially resolved by VLTI/AMBER spectro-interferometry

157 citations · 484 across the 9 of their papers we have counts for

collaborators

11 papers

astro-ph200827 cited

Characterization of integrated optics components for the second generation of VLTI instruments

S. Lacour, L. Jocou, T. Moulin +10

Two of the three instruments proposed to ESO for the second generation instrumentation of the VLTI would use integrated optics for beam combination. Several design are studied, inc…

astro-ph2008

System overview of the VLTI Spectro-Imager

L. Jocou, J. P. Berger, F. Malbet +30

The VLTI Spectro Imager project aims to perform imaging with a temporal resolution of 1 night and with a maximum angular resolution of 1 milliarcsecond, making best use of the Very…

astro-ph2008157 cited

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,…

astro-ph20087 cited

VSI: the VLTI spectro-imager

F. Malbet, D. Buscher, G. Weigelt +51

The VLTI Spectro Imager (VSI) was proposed as a second-generation instrument of the Very Large Telescope Interferometer providing the ESO community with spectrally-resolved, near-i…

astro-ph200833 cited

MWC 297: a young high-mass star rotating at critical velocity

B. Acke, T. Verhoelst, M. E. van den Ancker +9

MWC 297 is a young massive nearby B[e] star. The central star has a large projected rotational velocity of 350 km/s. Despite the wealth of published observations, the nature of thi…

astro-ph2008

Milli-arcsecond astrophysics with VSI, the VLTI spectro-imager in the ELT era

F. Malbet, D. Buscher, G. Weigelt +49

Nowadays, compact sources like surfaces of nearby stars, circumstellar environments of stars from early stages to the most evolved ones and surroundings of active galactic nuclei c…