Cohen et al. 1970

Cohen, J.M., W.D. Langer, L.C. Rosen, and A.G.W. Cameron, 1970: Neutron star models based on an improved equation of state. Astrophys. Space Sci., 6, 228-239, doi:10.1007/BF00651224.

Using an equation of state for cold degenerate matter which takes nuclear forces and nuclear clustering into account, neutron star models are constructed. Stable models were obtained in the mass range 0.065 M_☉ and density range 10^14.08 to 10^15.4 gm/cm³. All of these models were found to be bound. The outer crystalline layer of the star was found to have a thickness of 200m or more depending on the mass of the model.

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Cohen, J.M., Langer, W.D., Rosen, L.C., and Cameron, A.G.W.: Neutron star models based on an improved equation of state, Astrophys. Space Sci., 6, 228-239, doi:10.1007/BF00651224, 1970.

Cohen, J.M., W.D. Langer, L.C. Rosen, and A.G.W. Cameron (1970), Neutron star models based on an improved equation of state, Astrophys. Space Sci., 6, 228-239, doi:10.1007/BF00651224.

Cohen, J.M., W.D. Langer, L.C. Rosen, and A.G.W. Cameron, 1970: Neutron star models based on an improved equation of state. Astrophys. Space Sci., 6, 228-239, doi:10.1007/BF00651224.

Cohen, J.M., Langer, W.D., Rosen, L.C., & Cameron, A.G.W. 1970, Astrophys. Space Sci., 6, 228, doi:10.1007/BF00651224.

Cohen JM, Langer WD, Rosen LC, Cameron AGW. Neutron star models based on an improved equation of state, Astrophys Space Sci 1970;6:228-239. doi:10.1007/BF00651224.

J.M. Cohen, W.D. Langer, L.C. Rosen, A.G.W. Cameron, Astrophys. Space Sci. 6, 228-239, doi:10.1007/BF00651224 (1970).