activity
20032009
most citedParsec-scale dust distributions in Seyfert galaxies - Results of the MIDI AGN snapshot survey

129 citations · 321 across the 5 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2009129 cited

Parsec-scale dust distributions in Seyfert galaxies - Results of the MIDI AGN snapshot survey

Konrad R. W. Tristram, David Raban, Klaus Meisenheimer +11

The emission of warm dust dominates the mid-infrared spectra of active galactic nuclei (AGN). Only interferometric observations provide the necessary angular resolution to resolve…

astro-ph200820 cited

The close circumstellar environment of the semi-regular S-type star Pi^1 Gruis

Stéphane Sacuto, Alain Jorissen, Pierre Cruzalèbes +4

We study the close circumstellar environment of the nearby S-type star Pi^1 Gruis using high spatial-resolution, mid-infrared observations from the ESO/VLTI. Spectra and visibiliti…

astro-ph200754 cited

The molecular and dusty composition of Betelgeuse's inner circumstellar environment

Guy Perrin, Tijl Verhoelst, Stephen T. Ridgway +6

The study of the atmosphere of red supergiant stars in general and of Betelgeuse (alpha Orionis) in particular is of prime importance to understand dust formation and how mass is l…

astro-ph2007117 cited

Resolving the innermost parsec of Centaurus A at mid-infrared wavelengths

K. Meisenheimer, K. R. W. Tristram, W. Jaffe +11

We report the results of interferometric observations of Centaurus A with the MID-infrared Interferometer (MIDI) at ESO's VLTI telescope array. The interferometric measurements are…

astro-ph20061 cited

Study of the scientific potential of a three 40 cm Telescopes Interferometer at Dome C

B. Valat, F. X. Schmider, B. Lopez +4

Recent site testing (see: http://www-luan.unice.fr/Concordiastro/indexantartic.html) has shown that Dome C in Antarctica might have a high potential for stellar interferometry if s…

astro-ph2005

Extrasolar Planets with AMBER/VLTI, What can we expect from current performances ?

Florentin Millour, Martin Vannier, R. G. Petrov +2

We present the current performances of the AMBER / VLTI instrument in terms of differential observables (differential phase and differential visibility) and show that we are alread…