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1 Introduction
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2 Canonical two-fluid hydrodynamics
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3 Entrainment and effective masses
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4 Stationary two-fluid neutron star models
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5 The slow-rotation approximation
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6 Boundary conditions and integration constants
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7 Ellipticities, moments of inertia, and Kepler rotation rate
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8 An analytic solution
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9 Exploring the roles of relative rotation, entrainment and
"symmetry energy''
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10 Conclusions
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Appendix A: An alternative derivation of the first integrals of motion
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References
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