IMPETUS: New Cloudy's radiative tables for accretion onto a galaxy black
  hole
  We present digital tables for the radiative terms that appear in the energy
and momentum equations used to simulate the accretion onto supermassive black
holes (SMBHs) in the center of galaxies. Cooling and heating rates and
radiative accelerations are calculated with two different Spectral Energy
Distributions (SEDs). One SED is composed of an accretion disk +
[X-ray]-powerlaw, while the other is made of an accretion disk +
[Corona]-bremsstrahlung with $T_X=1.16 \times 10^8$ K, where precomputed
conditions of adiabatic expansion are included. Quantification of different
physical mechanisms at operation are presented, showing discrepancies and
similarities between both SEDs in different ranges of fundamental physical
parameters (i.e., ionization parameter, density, and temperature). With the
recent discovery of outflows originating at sub-parsec scales, these tables may
provide a useful tool to model gas accretion processes onto a SMBH.
