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Last name: MILLOUR
First name: F.
IAU Colloq. 200: Direct Imaging of Exoplanets: Science and Techniques, Cambridge University Press 1, pp. 291-296 (2006)
Proceedings of the Conference, LPI Contribution 1286, p. 8626 (2005)
We present the high angular resolution technique of colour-differential interferometry for direct detection of extrasolar giant planets (EGPs). The measurement of differential phase with long-baseline ground-based interferometers in the near-infrared could allow the observation of several hot giant extrasolar planets in tight orbit around the...
in Advances in Stellar Interferometry, eds. J. D. Monnier, M. Schöller and W. C. Danchi, SPIE 6269, p. 138 (2006)
n/a, eds. J. D. Monnier, M. Schöller and W. C. Danchi, SPIE n/a, (2006)
A handful of binary Wolf-Rayet stars are known to harbour spectacular spiral structures spanning a few hundred AU. These systems host some of the highest dust production rates in the Universe and are therefore interesting candidates to address the origin of the enigmatic dust excess observed across galactic evolution. The substantial...
Advances in Stellar Interferometry, eds. J. D. Monnier, M. Schoeller and W. C. Danchi, SPIE 6268, p. 626802 (2006)
Context. Canopus, the brightest and closest yellow supergiant to our Solar System, offers a unique laboratory for understanding the physics of evolved massive stars.Aims. We aim at quantitatively exploring a large space of fundamental parameters of Canopus based on the combined analysis of its spectral energy distribution (SED) and optical-IR...
Advances in Stellar Interferometry, eds. J. D. Monnier, M. Schoeller and W. C. Danchi, SPIE 6268, p. 626802 (2006)
n/a, EAS Publications Series 22, pp. 379-388 (2006)
Context. HD 110432 was classified as a "γ Cas X-ray analog" since it has similar peculiar X-ray and optical characteristics, i.e. a hard-thermal X-ray variable emission and an optical spectrum affected by an extensive disk. Lopes de Oliveira et al. (2007) suggest that it might be a Be star harboring an accreting white dwarf or that the X-rays...
Context. HD 110432 was classified as a "γ Cas X-ray analog" since it has similar peculiar X-ray and optical characteristics, i.e. a hard-thermal X-ray variable emission and an optical spectrum affected by an extensive disk. It might be a Be star harboring an accreting white dwarf or that the X-rays may come from an interaction between the...
International audience
The Messenger, 127, p. 37 (2007)
Astron. and Astroph., n/a, (2006)
Astron. & Astrophys., 464, pp. 59-71 (2007)
International audience