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The M82 galaxy has been the subject of several studies basically because itis relatively close to to the Milky Way and it displays a strong star formationactivity. Using multi-band images of M82 we have determined the age andextinction of the stellar population located in regions with strong UVemission, these region are in the nucleus and the disk of M82. We also haveemployed the UV images of M82 and the physical properties of its stellarclusters to measure the contribution of the clusters to the detected UV flux.We found that clusters located in the nuclear regions are emitting all theobserved UV flux, whereas clusters of the disk emit less than ~10%. Based onthe results obtained from this work we can infer that the field stars locatedin the disk of M82 could have been part of a stellar cluster when they wereborn.

Age and Extinction of the Ultraviolet Emitting Regions in M82