Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: 3D ISM-Shock Spectral Emission: X-ray models for Radio Galaxy SED
  Modeling   Galaxies form out of small fluctuations in a smoothly expanding Universe.
However, the initial gravitational collapse phase is accompanied by the
formation of supermassive black holes and clusters of massive stars. Black
holes and star clusters generate powerful outflows in the form of jets and
superwinds that interact with still infalling gas, possibly regulating the
galaxy formation process, initiating new sites of star formation, and carrying
chemically enriched gas to the intergalactic medium. Unfortunately, beyond this
qualitative description our detailed theoretical understanding is poor.
  New results from 3D simulations of a GPS/CSS galaxy, with gravitational
potentials included, shed some new light on the jet driven outflow process in
particular. New code capabilites to predict detailed X-ray spectra from
multi-dimensional time-dependent dynamics simulations of Galaxy Feedback, and
will be useful for future interpretation of X-ray and radio SEDs of forming
galaxies.

7
The categories of this paper are: hep-th
5
The categories of this paper are: gr-qc
32
The categories of this paper are: atom-ph
37
The categories of this paper are: supr-con
2
The categories of this paper are: math
27
The categories of this paper are: comp-gas
20
The categories of this paper are: acc-phys
29
The categories of this paper are: funct-an
36
The categories of this paper are: cmp-lg
30
The categories of this paper are: q-alg
8
The categories of this paper are: hep-ex
19
The categories of this paper are: eess
35
The categories of this paper are: mtrl-th
18
The categories of this paper are: econ
28
The categories of this paper are: alg-geom
17
The categories of this paper are: q-fin