The nearest ultra diffuse galaxy: UGC2162
  We describe the structural, stellar population and gas properties of the
nearest Ultra Diffuse Galaxy (UDG) discovered so far: UGC2162 (z=0.00392;
R$_{e,g}$=1.7$(\pm$0.2) kpc; $\mu_g(0)$=24.4$\pm$0.1 mag/arcsec$^2$;
g-i=0.33$\pm$0.02). This galaxy, located at a distance of 12.3($\pm$1.7) Mpc,
is a member of the M77 group. UGC2162 has a stellar mass of
$\sim$2($^{+2}_{-1}$)$\times$10$^7$ M$_\odot$ and is embedded within a cloud of
HI gas $\sim$10 times more massive: $\sim$1.9($\pm$0.6)$\times$10$^8$
M$_\odot$. Using the width of its HI line as a dynamical proxy, the enclosed
mass within the inner R$\sim$5 kpc is $\sim$4.6($\pm$0.8)$\times$10$^9$
M$_\odot$ (i.e. M/L$\sim$200). The estimated virial mass from the cumulative
mass curve is $\sim$8($\pm$2)$\times$10$^{10}$ M$_\odot$. Ultra-deep imaging
from the IAC Stripe82 Legacy Project show that the galaxy is irregular and has
many star forming knots, with a gas-phase metallicity around one-third of the
solar value. Its estimated Star Formation Rate (SFR) is $\sim$0.01
M$_\odot$/yr. This SFR would double the stellar mass of the object in $\sim$2
Gyr. If the object were to stop forming stars at this moment, after a passive
evolution, its surface brightness would become extremely faint:
$\mu_g(0)$$\sim$27 mag/arcsec$^2$ and its size would remain large
R$_{e,g}$$\sim$ 1.8 kpc. Such faintness would make it almost undetectable to
most present-day surveys. This suggests that there could be an important
population of M$_{\star}$$\sim$10$^7$ M$_\odot$ "dark galaxies" in rich
environments (depleted of HI gas) waiting to be discovered by current and
future ultra-deep surveys.
