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  • Initial mass function biase...
    Apellaniz, Jesus Maiz

    Astrophysics and space science, 12/2009, Letnik: 324, Številka: 2-4
    Journal Article

    I discuss two of the possible sources of biases in the determination of the stellar initial mass function: binning and the existence of unresolved components. The first source is important for clusters with a small number of stars detected in a given mass bin, while the second is relevant for all clusters located beyond the immediate solar neighborhood. For both cases I present results of numerical simulations, and I discuss strategies to correct for their effects. I also present a brief description of a third unrelated bias source.