Spectrally resolved interferometry of luminous and multiple stars with the GI2T

Details Spectrally resolved interferometry of luminous and multiple stars with the GI2T Spectrally resolved interferometry of luminous and multiple stars with the GI2T

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998spie.3350..505t&link_type=abstract

Proc. SPIE Vol. 3350, p. 505-516, Astronomical Interferometry, Robert D. Reasenberg; Ed.

Physics

1

Scientific paper

This paper reviews the scientific results obtained with the Grand Interferometer a 2 Telescopes (GI2T) from 1990 to 1996. During this epoch, accurate spectroscopy coupled to interferometry were achieved on luminous and multiple stars. Subtle structures in circumstellar environments such as: jets in the binary system (beta) Lyrae, clumpiness in the wind of P Cygni, a rotating arm in (zetz) Cas models. In addition to GI2T results, we develop in our group hydrodynamic and radiative transfer models dedicated to the interpretation of interferometry results. These models can directly constrain luminous star physics through their observable parameters.

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