The effective temperatures and the bolometric corrections of 0-G type stars and derived from de-reddened monochrometric and integrated fluxes obtained by absolute spectrophotometry on the ground and satellite (IUE, 1985, OAO : Code and Meade, 1979 ; Code et al., 1980), using the method simillar to that of Code et al.(1976) with the LTE model atmospheres by Kurucz(1979). The effective temperatures and the bolometric corrections derived from this work are found to be in good agreement with those of Code et al. (1976), Morossi and Malagnini (1985), Malagnini et al. (1985) etc., being significant for basic astrophysical quantities.

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