Abstract:
The continuum energy distributions of six Be stars, namely 25 Cyg, 31 Peg, HR 8758, 14 Lac, 12 Vul and β Psc in the wavelength region λ λ3200-7800 Å, are presented. Comparing the observed energy distributions with those of theoretical models given by Kurucz (1979), their effective temperatures are determined. A near-infrared excess emission at wavelengths above λ6000 Å is seen in most of the stars.
