Active hot star shells

Astronomy and Astrophysics – Astrophysics

Scientific paper

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&Gamma, Cas, &Phis, Per, &Psi, Per, &Eta, Tau, 48 Per, &Zeta, Tau, &Beta, Cmi, &Beta, Lyr Interferometry, Visibility, Angular Diameter, Gi2T/Regain, Mkiii

Scientific paper

Interferometry in the visible provides milliarcsecond spatial resolution and thus has been used for studying the circumstellar environment of active hot stars. In this paper I will illustrate how the visibility modulus and phase can be used to better constrain the physics of Be disks through results from the VLA, the MkII and the GI2T interferometers. I will insist on the importance and the potential of coupling high angular resolution with high spectral resolution to the study of Be shells. Finally I will present a possible study of the circumstellar disk of Be stars using the VLTI.

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