Abstract
We have derived the normal spectral energy distributions for those early-type subgiants, giants, and supergiants that were not investigated in our earlier studies, which were in most cases also not included in the studies of Sviderskiene. Color indices computed using our normal energy distributions are in good agreement with normal colors derived from observations in the Vilnius photometric system. The reliability of our distribution curves is also demonstrated by comparisons of observed and computed (W-B)-(B-V) two-color diagrams in the WBVR system. Normal color indices for the photometric WBVR system are derived.
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