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Chapter and Conference Paper
A Radiative Wind Model for Active Hot Stars
Radiative wind from active hot stars has been studied for more than two decades. During this period, numerous models which try to fit a small number of observables as closely as possible have been developed, s...
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Chapter and Conference Paper
Physics of radiatively driven winds by high angular resolution observations (HARO)
Numerous models have been developed during the last two decades which try to fit a small number of “classical” observables as closely as possible (i.e Hα line profile and continuum energy distribution or polar...
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Chapter
Sub-Milliarcsecond Structures in P Cyg
We report the first resolution of the envelope of P Cyg in Ha using the GI2T spectro-interferometer in the southern France. We detected a localized asymmetry at .8 mas to the South of P Cyg’s photosphere on Au...
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Chapter and Conference Paper
Stellar Astrophysics with Sub-Milliarcsecond Optical Interferometry
Although stellar interferometers are capable of measuring the angular diameters of stars, with longer baselines they may also be used to measure brightness variations across a star’s surface and to provide con...
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Chapter and Conference Paper
The Extended Hα Component of T Tau
We report the observation of T Tau by visible speckle interferometry at the CFHT. The observations were carried out at two wavelengths simultaneously. Each image was split into two, allowing improved data proc...
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Chapter and Conference Paper
Progress on GI2T
The purpose of this paper is to describe the operation of GI2T, the visible Michelson stellar interferometer with two 1.5 m apertures, as well as a presentation of its desired evolution.
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Chapter and Conference Paper
First Results of an International Multisite Multitechnique Campaign on omicron and
Omicron Andromedae is a multiple system of at least four stars: a B ↔Be star (component A), a spectroscopic binary (components B1-B2) and a close companion (component a). According to several studies (see Hill...
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Chapter and Conference Paper
Lock-In Image Subtraction: Detectability of Circumstellar Planets with the Large Space Telescope
Faint circumstellar features in the close vicinity of stars or qso’s are of considerable astrophysical interest since they can provide important informations on stellar parameters and evolutions: stellar compa...