To outline the position of the Local Void on the sky, we reproduce in
Fig. 1 the distribution of galaxies with known corrected radial velocities
V0 < 1500 km s-1 in a
region RA = [10.0, 23.5], D = [-20, +60]
. The 19
nearest galaxies with V0 < 750 km s-1 are shown as larger open
circles. The radial velocities were taken from the PGC catalogue (Paturel
et al. 1992) and updated with data from recent publications. The curves
correspond to the Milky Way avoidance zone within galactic latitudes +10
and
. As it can be seen from Fig. 1, inside a circle of 60
diameter around a point of {RA = 18
,
}
there is no galaxy having a radial velocity V0 < 1500 km s-1.
Searches for new nearby galaxies in the most obscured part of this area
undertaken by Nakanishi et al. (1997) among the IRAS sources, as well for
HI-rich dwarf galaxies (Hoffman et al. 1992), added nothing within the
drawn circle.
The distribution of more distant galaxies in the same sky region is shown
in Fig. 2. The first galaxies inside the Local Void zone appear just beyond
V0 = 1500 km s-1. Adopting for the Hubble parameter H = 75
km s-1/Mpc, we find that the empty volume is Mpc3.
It should be emphasized that there is still no systematic search for nearby dwarf galaxies in the whole Local Void area. Therefore, the possibility for such a large volume to be completely devoided of galaxies remains unproved. In the next section we describe the results of a special survey for nearby dwarf galaxy candidates on almost the whole area of the Local Void.
Copyright The European Southern Observatory (ESO)