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Initial mass function biases created by binning and unresolved systems

机译:由合并和未解决的系统产生的初始质量函数偏差

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摘要

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.
机译:在确定恒星初始质量函数时,我讨论了两种可能的偏差来源:装仓和未解决组分的存在。第一个来源对于在给定质量仓中检测到少量恒星的星团很重要,而第二个来源与位于紧邻太阳附近的所有星团都很重要。对于这两种情况,我都会给出数值模拟的结果,并讨论纠正其影响的策略。我还简要介绍了第三个不相关的偏见来源。

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