Bibcode
Kroupa, P.; Weidner, C.
Bibliographical reference
The Initial Mass Function 50 years later. Edited by E. Corbelli and F. Palle, INAF Osservatorio Astrofisico di Arcetri, Firenze, Italy; H. Zinnecker, Astrophysikalisches Potsdam, Germany. Astrophysics and Space Science Library Volume 327. Published by Springer, Dordrecht, 2005, p.175
Advertised on:
1
2005
Citations
10
Refereed citations
8
Description
(abridged) The {stellar IMF} has been found to be essentially invariant.
While some apparent differences are seen, the uncertainties inherent to
this game do not allow a firm conclusion to be made that the IMF varies
systematically with conditions. The IMF integrated over entire galaxies,
however, is another matter. Chemical and photometric properties of
various galaxies do hint at {galaxial IMFs} being steeper than the
stellar IMF, as is also deduced from direct star-count analysis in the
MW. These results are sensitive to the modelling of stellar populations
and to corrections for stellar evolution, and are thus also uncertain.
However, by realising that galaxies are made from dissolving star
clusters, star clusters being viewed as {the fundamental building blocks
of galaxies}, the result is found that galaxial IMFs must be
significantly steeper than the stellar IMF, because the former results
from a folding of the latter with the star-cluster mass function.
Furthermore, this notion leads to the important insight that galaxial
IMFs must vary with galaxy mass, and that the galaxial IMF is a strongly
varying function of the star-formation history for galaxies that have
assembled only a small mass in stars. Cosmological implications of this
are discussed.