Be stars

Low resolution observations of Be-stars type. For a description of Be phenomena and a view of my high spectral resolution monitoring of this stars, click here.

The spectral data were reduced in the standard manner using Iris and VisualSpec. The instrumental response function was removed from target spectra by using standard star spectra. The relative flux is normalized at the wavelength 6630 angstroms. Click here for a description of the spectrograph used. 

Gamma Cas