International audience
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November 2013 (v1)Journal articleUploaded on: December 3, 2022
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August 2008 (v1)Journal article
Context: We present the first high spatial-resolution monitoring of the dust-forming nova V1280 Sco, performed with the Very Large Telescope Interferometer (VLTI). Aims: These observations promise to improve the distance determination of such events and constrain the mechanisms leading to very efficient dust formation under the harsh physical...
Uploaded on: December 4, 2022 -
March 2007 (v1)Journal article
Aims.We report on spectrally dispersed interferometric AMBER/VLTI observations of the recurrent nova RS Oph five days after the discovery of its outburst on 2006 Feb. 12. Methods: Using three baselines ranging from 44 to 86 m, and a spectral resolution of λ/δλ=1500, we measured the extension of the milliarcsecond-scale emission in the K band...
Uploaded on: March 25, 2023 -
October 2016 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
2006 (v1)Conference paper
Advances in Stellar Interferometry, eds. J. D. Monnier, M. Schöller and W. C. Danchi, SPIE 6268, (2006)
Uploaded on: December 4, 2022 -
October 2016 (v1)Journal article
Context. The mass loss from massive stars is not understood well. η Carinae is a unique object for studying the massive stellar wind during the luminous blue variable phase. It is also an eccentric binary with a period of 5.54 yr. The nature of both stars is uncertain, although we know from X-ray studies that there is a wind-wind collision...
Uploaded on: December 3, 2022 -
August 2021 (v1)Journal article
Context. Carbon is one of the most abundant components in the Universe. While silicates have been the main focus of solid phase studies in protoplanetary discs (PPDs), little is known about the solid carbon content especially in the planet-forming regions (~0.1–10 au). Fortunately, several refractory carbonaceous species present C-H bonds (such...
Uploaded on: December 4, 2022