The Initial Mass Function in the ELT era

TL;DR

This paper discusses how upcoming extremely large telescopes will enhance our understanding of the initial mass function (IMF) by enabling observations of fainter and more compact stellar clusters, addressing key questions about its universality and environmental dependence.

Contribution

The paper evaluates the potential of future ELT observations to significantly improve knowledge of the IMF and address fundamental questions about its constancy and universality.

Findings

Future telescopes will observe fainter, more compact clusters.

Enhanced observations will help answer if the IMF is environment-dependent.

Improved data will clarify the universality of the IMF.

Abstract

The initial mass function (IMF) is an important, yet enigmatic aspect of the star formation process. The two major open questions regarding the IMF are: is the IMF constant regardless of environment? Is the IMF a universal property of star formation? The next generation of extremely large telescopes will allow us to observe further, fainter and more compact stellar clusters than is possible with current facilities. In these proceeding we present our study looking at just how much will these future observatories improve our knowledge of the IMF.