  This paper presents Very Long Baseline Array (VLBA) observations of 13
double-peaked [O III] emission-line type-2 Active Galactic Nuclei (AGNs) at
redshifts 0.06 < z < 0.41 (with a median redshift of z~0.15) identified in the
Sloan Digital Sky Survey. Such double-peaked emission-line objects may result
from jets or outflows from the central engine or from a dual AGN. The VLBA
provides an angular resolution of <~10 pc at the distance of many of these
galaxies, sufficient to resolve the radio emission from extremely close dual
AGNs and to contribute to understanding the origin of double-peaked [O III]
emission lines. Of the 13 galaxies observed at 3.6 cm (8.4 GHz), we detect six
at a 1\sigma\ sensitivity level of ~0.15 mJy/beam, two of which show clear jet
structures on scales ranging from a few milliarcseconds to tens of
milliarcseconds (corresponding to a few pc to tens of pc at a median redshift
of 0.15). We suggest that radio-loud double-peaked emission-line type-2 AGNs
may be indicative of jet produced structures, but a larger sample of
double-peaked [O III] AGNs with high angular resolution radio observations will
be required to confirm this suggestion.
