What does the IMF really tell us about star formation?

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics

Scientific paper

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To be published in the proceedings of IAU Symposium 262 "Stellar Populations - Planning for the Next Decade"

Scientific paper

Obtaining accurate measurements of the initial mass function (IMF) is often considered to be the key to understanding star formation, and a universal IMF is often assumed to imply a universal star formation process. Here, we illustrate that different modes of star formation can result in the same IMF, and that, in order to truly understand star formation, a deeper understanding of the primordial binary population is necessary. Detailed knowledge on the binary fraction, mass ratio distribution, and other binary parameters, as a function of mass, is a requirement for recovering the star formation process from stellar population measurements.

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