Properties of the most metal-poor gas-rich LSB dwarf galaxies SDSS
  J0015+0104 and J2354-0005 residing in the Eridanus void
  SDSS J0015+0104 is the lowest metallicity low surface brightness dwarf (LSBD)
galaxy known. The oxygen abundance in its HII region SDSS J001520.70+010436.9
(at ~1.5 kpc from the galaxy centre) is 12+log(O/H)=7.07 (Guseva et al.). This
galaxy, at the distance of 28.4 Mpc, appears to reside deeply in the volume
devoid of luminous massive galaxies, known as the Eridanus void. SDSS
J235437.29-000501.6 is another Eridanus void LSBD galaxy, with parameter
12+log(O/H)=7.36 (also Guseva et al.). We present the results of their HI
observations with the Nancay Radio Telescope revealing their high ratios of
M(HI)/L_B ~2.3. Based on the Sloan Digital Sky Survey images, we derived for
both galaxies their radial surface brightness profiles and the main photometric
parameters. Their colours and total magnitudes are used to estimate the galaxy
stellar mass and ages. The related gas mass-fractions, f_g ~0.98 and ~0.97, and
the extremely low metallicities (much lower than for their more typical
counterparts with the same luminosity) indicate their unevolved status. We
compare these Eridanus void LSBDs with several extreme LSBD galaxies residing
in the nearby Lynx-Cancer void. Based on the combination of all their unusual
properties, the two discussed LSBD galaxies are similar to the unusual LSBDs
residing in the closer void. This finding presents additional evidence for the
existence in voids of a4 figures, sizable fraction of low-mass unevolved
galaxies. Their dedicated search might result in the substantial increase of
the number of such objects in the local Universe and in the advancement of
understanding their nature.
