693.932 PEOPLE
| People | Locations | Statistics |
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| Naji, M. |
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| Motta, Antonella |
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| Aletan, Dirar |
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| Mohamed, Tarek |
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| Ertürk, Emre |
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| Taccardi, Nicola |
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| Kononenko, Denys |
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| Petrov, R. H. | Madrid |
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| Alshaaer, Mazen | Brussels |
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| Bih, L. |
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| Casati, R. |
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| Muller, Hermance |
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| Kočí, Jan | Prague |
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| Šuljagić, Marija |
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| Kalteremidou, Kalliopi-Artemi | Brussels |
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| Azam, Siraj |
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| Ospanova, Alyiya |
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| Blanpain, Bart |
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| Ali, M. A. |
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| Popa, V. |
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| Rančić, M. |
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| Ollier, Nadège |
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| Azevedo, Nuno Monteiro |
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| Landes, Michael |
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| Rignanese, Gian-Marco |
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Weigelt, G.
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (12/12 displayed)
- 2024Chromatically modeling the parsec-scale dusty structure in the center of NGC 1068citations
- 2022Locating dust and molecules in the inner circumstellar environment of R Sculptoris with MATISSEcitations
- 2022MATISSE first pictures of dust and molecules around R Sculptoriscitations
- 2021First MATISSE L -band observations of HD 179218:Is the inner 10 au region rich in carbon dust particles?citations
- 2021First MATISSE L -band observations of HD 179218. Is the inner 10 au region rich in carbon dust particles? ; First MATISSE L -band observations of HD 179218. Is the inner 10 au region rich in carbon dust particles?: Is the inner 10 au region rich in carbon dust particles?citations
- 2021First MATISSE L-band observations of HD,179218. Is the inner 10~au region rich in carbon dust particles?
- 2007VLTI/MIDI Observation of the Silicate Carbon Star IRAS 08002--3803: Dusty Environment Spatially Resolved for the First Time
- 2007Temporal variations of the outer atmosphere and the dust shell of the carbon-rich Mira variable V Ophiuchi probed with VLTI/MIDIcitations
- 2007The innermost region of AGN tori: implications from the HST/NICMOS type 1 point sources and near-IR reverberationcitations
- 2006Near-infrared speckle interferometry and radiative transfer modelling of the carbon star LP Andromedaecitations
- 2006High angular resolution N-band observation of the silicate carbon star IRAS08002-3803 with the VLTI/MIDI instrument . Dusty environment spatially resolvedcitations
- 2001Structure and physical properties of the rapidly evolving dusty envelope of <ASTROBJ>IRC +10 216</ASTROBJ> reconstructed by detailed two-dimensional radiative transfer modelingcitations
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