GCAS_1.DAT
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.
