  In this work, we get an idea of the existence of compact stars in the
background of f(T) modified gravity where T is a scalar torsion. We acquire the
equations of motion using anisotropic property within the spherically compact
star with electromagnetic field, quintessence field and modified Chaplygin gas
in the framework of modified f(T) gravity. Then by matching condition, we
derive the unknown constants of our model to obtain many physical quantities to
give a sketch of its nature and also study anisotropic behavior, energy
conditions and stability. Finally, we estimate the numerical values of mass,
surface redshift etc from our model to compare with the observational data for
different types of compact stars.
