Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: The role of the Initial Mass Function in modelling the Intra-Cluster
  Medium   The expected metal enrichment of the intra-cluster medium (ICM) and the
partition of metals between cluster galaxies and the hot ICM depends on the
stellar Initial Mass Function (IMF). The choice of the IMF in simulations of
clusters has also important consequences on the "cold fraction", which is a
fundamental constraint on cluster physics.
  We discuss the chemical enrichment and the cold fraction in clusters as
predicted with different IMFs, by means of a straightforward approach that is
largely independent of the details of chemical evolution models or simulations.
We suggest this simple approach as a guideline to select the input parameters
and interpret the results of more complex models and hydrodynamical
simulations.

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The categories of this paper are: q-fin
10
The categories of this paper are: q-bio
30
The categories of this paper are: q-alg
15
The categories of this paper are: nucl-ex
26
The categories of this paper are: bayes-an
3
The categories of this paper are: physics
32
The categories of this paper are: atom-ph
0
The categories of this paper are: hep-ph
1
The categories of this paper are: cs
8
The categories of this paper are: hep-ex
36
The categories of this paper are: cmp-lg
11
The categories of this paper are: hep-lat
34
The categories of this paper are: chem-ph
9
The categories of this paper are: nlin
24
The categories of this paper are: dg-ga
13
The categories of this paper are: quant-ph