Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: AGN feedback using AMR cosmological simulations   Feedback processes are thought to solve some of the long-standing issues of
the numerical modelling of galaxy formation: over-cooling, low angular
momentum, massive blue galaxies, extra-galactic enrichment, etc. The accretion
of gas onto super-massive black holes in the centre of massive galaxies can
release tremendous amounts of energy to the surrounding medium. We show, with
cosmological Adaptive Mesh Refinement simulations, how the growth of black
holes is regulated by the feedback from Active Galactic Nuclei using a new dual
jet/heating mechanism. We discuss how this large amount of feedback is able to
modify the cold baryon content of galaxies, and perturb the properties of the
hot plasma in their vicinity.

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The categories of this paper are: mtrl-th
13
The categories of this paper are: quant-ph
17
The categories of this paper are: q-fin
15
The categories of this paper are: nucl-ex
18
The categories of this paper are: econ
21
The categories of this paper are: adap-org
34
The categories of this paper are: chem-ph
28
The categories of this paper are: alg-geom
26
The categories of this paper are: bayes-an
33
The categories of this paper are: plasm-ph
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The categories of this paper are: atom-ph
11
The categories of this paper are: hep-lat
14
The categories of this paper are: math-ph
24
The categories of this paper are: dg-ga
2
The categories of this paper are: math
19
The categories of this paper are: eess