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- W197237455 abstract "Abstract Interferometry in the visible now provides milliarcsecond spatial resolution and thus can be used for studying the circumstellar environment of Be stars. In this review I will first introduce the two basic quantities that an interferometer can access: the modulus and the phase of the visibility. I will illustrate how these two quantities can be used to understand the physics of Be disks through recent 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 disks. Since the possibility of direct optical imaging of Be disks will be limited due to complexity and time consumption, I will present the role models can play in interpreting high angular resolution observations when direct imaging become difficult. Finally I will draw up a list of challenging objectives for the next generation of synthetic arrays (GI2T/REGAIN, Keck, ST3, VLTI) which will bring new understanding of active hot stars physics." @default.
- W197237455 created "2016-06-24" @default.
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- W197237455 date "2000-01-01" @default.
- W197237455 modified "2023-09-25" @default.
- W197237455 title "Direct Optical Imaging of Be Disks" @default.
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- W197237455 doi "https://doi.org/10.1017/s0252921100055743" @default.
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