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We analyse a feature that is detectable at the differential phases ofhigh-resolution spectro-interferometry of Be stars. The origin of this feature(dubbed CQE-PS, Central Quasi Emission Phase Signature) lies in thedifferential absorption of photospheric radiation by the circumstellar disk,which is spectroscopically detected as a CQE line profile in shell stars. Thisphenomenon has great diagnostic potential for Be star disks, revealingproperties of these disks on the scale of a few stellar radii.

On the CQE Phase Signature Feature in High-Resolution Spectro-Interferometry of Be Stars