The masses of open star clusters and their tidal tails and the stellar initial mass function

Open Access

Fig. 2

MLR used in this work. The absolute V-band magnitudes of stars, M_V, are shown in relation to their stellar mass, m. The red dots show the data points from Kroupa et al. (1993), while the grey line shows the fit used for m > 1.5 M_⊙.

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