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Fig. 7.


MV/(BV)0 diagram for likely members of NGC 3105. Stars observed spectroscopically are represented in red. Spectral types for the brightest stars are marked. Blue circles are the rest of the early members found photometrically. The black line shows, as a ZAMS, a PARSEC isochrone of 10 Ma computed at the cluster metallicity. The best-fitting yields a distance modulus of μ = 14.3 ± 0.2.

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