Abstract
We have compared the results of multicolor U BV R and Hα photometry for 169 young star-formation complexes in five galaxies using a grid of evolutionary models for young star clusters. The ages and interstellar absorptions are estimated for 102 star-formation complexes with the standard uncertainties σt = 0.30 dex and \( \sigma _{A_V } = 0.45^m \). The accuracies of these parameters were verified using numerical simulations.
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