  This article primarily investigates the existence of the charged compact star
under the conformal motion treatment within the context of f(Q) gravity. We
have developed two models by implementing the power-law and linear form of
conformal factor, enabling an in-depth comparison in our study. We have
selected the MIT Bag model equation of state to describe the connection between
pressure and energy density and matched the interior spherically symmetric
space-time with the Bardeen space-time. In addition, the present research
examines various physically valid characteristics of realistic stars, such as
PSR J1614-2230, PSR J1903+327, Vela X-1, Cen X-3, and SMC X-1. We compare two
constructed models by attributing the behavior of density, pressure,
equilibrium conditions, and the adiabatic index. We have additionally included
a brief analysis of the scenario involving Reissner-Nordstrom spacetime as an
external geometry for the matching condition. In contrast to the
Reissner-Nordstrom instance, the Bardeen model with the extra term in the
asymptotic representations yields a more intriguing and viable result. The
current analysis reveals that the resulting compact star solutions are
physically acceptable and authentic when considering the presence of charge
with conformal motion in f(Q) gravity.
