  Compact stars have long served as a test bed of gravitational models and
their coupling with stellar matter. In this work, we explore the behavior of an
exponential model in f(T) gravity through the Tolman-Oppenheimer-Volkoff
equation. This is performed for different envelope thicknesses. Finally,
constraints on the models parameters are obtained, which are comparable to the
results obtained using cosmological survey data. This consistency across the
strong astrophysical and weak cosmological scales shows reasonable viability of
the underlying model.
