  Massive galaxies are expected to grow through different transformative
evolutionary phases where high-redshift starburst galaxies and quasars are
examples of such phases. The physical mechanisms driving these phases include
companion galaxy interactions, active galactic nuclei feedback, and magnetic
fields. Our aim is to characterize the physical properties and the environment
of the submillimeter galaxy AzTEC-3 at z = 5.3 and the lensed quasar BRI
0952-0115 at z = 4.4, to set a limit on the polarization properties, as well as
placing both in the broader context of galaxy evolution. We used full
polarization, sub-arcsecond-resolution, ALMA band-7 observations of both BRI
0952-0115 and AzTEC-3 and detect [CII] line emission towards both galaxies,
along with companions in each field. We present an updated gravitational
lensing model for BRI 0952-0115. We present infrared luminosities,
star-formation rates, and [CII] line to infrared luminosity ratios for each
source. The [CII] emission line profile for both BRI 0952-0115 and AzTEC-3
exhibit a broad, complex morphology, indicating the possible presence of
outflows. We present evidence of a 'gas bridge' between AzTEC-3 and a companion
source. Using a simple dynamical mass estimate for the sources, we suggest that
both systems are undergoing minor or major mergers. No polarization is detected
for the [CII], placing an upper limit below that of theoretical predictions.
Our results show that high-velocity wings are detected, indicating possible
signs of massive outflows; however, the presence of companion galaxies can
affect the final interpretation. Furthermore, the results provide additional
evidence in support of the hypothesis that massive galaxies form in overdense
regions, growing through interactions. Finally, strong, ordered magnetic fields
are unlikely to exist at the kiloparsec scale in the two studied sources.
