SCYON Abstract

Received on May 6 2009

What does a universal IMF imply about star formation?

AuthorsSimon P. Goodwin and M.B.N. Kouwenhoven
AffiliationThe University of Sheffield, UK
Accepted byMonthly Notices of the Royal Astronomical Society
Contacts.goodwin@sheffield.ac.uk

t.kouwenhoven@sheffield.ac.uk
URLhttp://arxiv.org/abs/0904.4619
Links

Abstract

We show that the same initial mass function (IMF) can result from very different modes of star formation from very similar underlying core and/or system mass functions. In particular, we show that the canonical IMF can be recovered from very similar system mass functions, but with very different mass ratio distributions within those systems. This is a consequence of the basically log-normal shapes of all of the distributions. We also show that the relationships between the shapes of the core, system, and stellar mass functions may not be trivial. Therefore, different star formation in different regions could still result in the same IMF.