  The Green Bank Telescope (GBT) Diffuse Ionized Gas Survey (GDIGS) traces
ionized gas in the Galactic midplane by observing radio recombination line
(RRL) emission from 4-8 GHz. The nominal survey zone is $32.3^{\circ}> {\ell} >
-5^{\circ}$, $|b|<0.5^{\circ}$. Here, we analyze GDIGS Hn${\alpha}$ ionized gas
emission toward discrete sources. Using GDIGS data, we identify the velocity of
35 H II regions that have multiple detected RRL velocity components. We
identify and characterize RRL emission from 88 H II regions that previously
lacked measured ionized gas velocities. We also identify and characterize RRL
emission from eight locations that appear to be previously-unidentified H II
regions and 30 locations of RRL emission that do not appear to be H II regions
based on their lack of mid-infrared emission. This latter group may be a
compact component of the Galactic Diffuse Ionized Gas (DIG). There are an
additional 10 discrete sources that have anomalously high RRL velocities for
their locations in the Galactic plane. We compare these objects' RRL data to
13CO, H I and mid-infrared data, and find that these sources do not have the
expected 24 ${\mu}$m emission characteristic of H II regions. Based on this
comparison we do not think these objects are H II regions, but we are unable to
classify them as a known type of object.
