The nearest ultra diffuse galaxy: UGC2162
arXiv:1701.03804 · doi:10.3847/1538-4357/aa5cbb
Abstract
We describe the structural, stellar population and gas properties of the nearest Ultra Diffuse Galaxy (UDG) discovered so far: UGC2162 (z=0.00392; R=1.70.2) kpc; =24.40.1 mag/arcsec; g-i=0.330.02). This galaxy, located at a distance of 12.3(1.7) Mpc, is a member of the M77 group. UGC2162 has a stellar mass of 2()10 M and is embedded within a cloud of HI gas 10 times more massive: 1.9(0.6)10 M. Using the width of its HI line as a dynamical proxy, the enclosed mass within the inner R5 kpc is 4.6(0.8)10 M (i.e. M/L200). The estimated virial mass from the cumulative mass curve is 8(2)10 M. 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 0.01 M/yr. This SFR would double the stellar mass of the object in 2 Gyr. If the object were to stop forming stars at this moment, after a passive evolution, its surface brightness would become extremely faint: 27 mag/arcsec and its size would remain large R 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 M10 M "dark galaxies" in rich environments (depleted of HI gas) waiting to be discovered by current and future ultra-deep surveys.
5 pages; 3 figures, accepted for publication in ApJ; minor changes to match the published version
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