  The latest High Altitude Water Cherenkov (HAWC) point-like source catalog up
to 56 TeV reported the detection of two sources in the region of the Galactic
plane at galactic longitude 52\deg < l < 55\deg, 3HWC J1930+188 and 3HWC
J1928+178. The first one is associated with a known TeV source, the supernova
remnant SNR G054.1+00.3. It was discovered by one of the currently operating
Imaging Atmospheric Cherenkov Telescope (IACT), the Very Energetic Radiation
Imaging Telescope Array System (VERITAS), detected by the High Energy
Stereoscopic System (H.E.S.S.), and identified as a composite SNR. However, the
source 3HWC J1928+178, discovered by HAWC and coincident with the pulsar PSR
J1928+1746, was not detected by any IACT despite their long exposure on the
region, until a recent new analysis of H.E.S.S. data was able to confirm it.
Moreover, no X-ray counterpart has been detected from this pulsar. We present a
multicomponent fit of this region using the latest HAWC data. This reveals an
additional new source, HAWC J1932+192, which is potentially associated with the
pulsar PSR J1932+1916, whose gamma-ray emission could come from the
acceleration of particles in its pulsar wind nebula. In the case of 3HWC
J1928+178, several possible explanations are explored, in a attempt to unveil
the origins of the very-high-energy gamma-ray emission.
