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In the present paper, we have investigated magnetized LRS Bianchi type-I massive string cosmological model for perfect fluid distribution with cosmological term . To obtain the explicit solution of the model we suppose expansion is propotional to the shear and is inversely proportional to , where R is scale factor under two cases: (i) and (ii) where and are proper energy density and string tension density respectively. We have also discussed physical and geometrical characteristics of thedoi:10.26438/ijsrpas/v7i3.167172 fatcat:jabxvflnmfc6tc3gpruwh2vty4