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Estimating interstellar extinction towards elliptical galaxies and star clusters

We used the catalog with 402 elliptical galaxies compiled by Burstein (2003) which contains the E(B-V) determined by Burstein & Heiles (1978,1982, BH) and Schlegel et al. (1998, SFD) methods. The figure 3 presents the comparisons of the Model A using two zero point definitions: (BH:SFD-0.016) and (SFD:BH+0.019), respectively. The Table 2 shows the rms values obtained in these comparisons. V. Comparison with star clusters