The contribution of galaxies to OMEGA_0

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We estimate the contribution of galaxies to the cosmological density Omega_0 including also their extended dark halos. We find Omega_gal< 0.1, so implying that the matter in galaxies cannot by itself close the Universe but marginally could be baryonic. (latex file)two figures available upon request).
4 pages, preprint SISSA, 24/94/A

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