IMF biases created by binning and unresolved systems


J. Maíz Apellániz

IAA-CSIC

I discuss two of the possible sources of biases in the determination of the IMF: 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 one is relevant for all clusters located beyond the immediate solar neighborhood. For both cases I will present results of numerical simulations and I will discuss strategies to correct for their effects. I also present a brief description of a third unrelated bias source.

Reference: To appear in "Young massive clusters, initial conditions and environments"
Status: Conference proceedings

Weblink: http://arxiv.org/abs/0801.3778

Comments:

Email: jmaiz@iaa.es