On the Generalized-Faber Jackson relation for NGC 1052 DF2 galaxy
  The conjectures of Hawking-Bekenstein of that gravity and temperature are
closely related, was the beginning of the formulation of thermodynamic models
of gravity. Using one of these models, we show that the thermal bath
temperature of NGC1052-DF2 dwarf galaxy is about 6.5 K higher than the
temperature of the thermal bath of the local dwarf galaxies. We claim that this
temperature difference is responsible by the behavior of the NGC1052-DF2 galaxy
to be apparently a galaxy with lack dark matter. This difference arises due to
that the host galaxy of NGC1052-DF2, the elliptic galaxy NGC1052 is a
LINER-type active galactic nucleus, with signals the intense starburst activity
in the galaxy's center. Debye Gravitational Theory (DGT), allows obtaining a
Generalized Faber-Jackson relation to described the dwarf galaxies and
obtaining the velocity dispersion as a function of thermal bath temperature.
DGT predict a velocity dispersion to NGC1052-DF2 dwarf galaxy in agreement with
the very-low values reported in the literature. Also, DGT predicts that
several, or maybe all dwarf galaxies from NGC1052 must have the same behavior
than NGC1052-DF2 because they are immersed in thermal baths almost with the
same temperature, this behavior already was observed in a second galaxy, the
NGC1052-DF4 dwarf galaxy. Also, DGT predicts the same behavior, in all
satellite galaxies orbiting galaxies with active nuclei.
