Abstract:
The continuum energy distribution data of ten Be stars - namely, HR 1761, HR 1786, HR 1820, σOri, ω Ori, OT Gem, β Lyr, HR 7983, νCyg, and 59 Cyg- have been presented in the wavelength range λλ3200-8000 Å. The observed energy distribution curve shows near infrared excess for majority of Be stars and a double Balmer jump for HR 8047 and HR 8146. Empirical effective temperatures of these stars have been estimated by comparing the observed continuum energy distribution with that of computed theoretical models given by Kurucz (1979).
