Some Bianchi type III cosmological models with magnetic field for massive string are investigated. F 12 is only the non-vanishing component of electromagnetic field tensor F i j . To get a determinate solution. we have assumed that the expansion (θ) in the model is proportional to the shear (σ). This leads to C = A n where A and C are functions of time alone. A particular solution for n = 1 is discussed. The physical implications of the models, are also discussed.
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