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

Copyright ESO 2002
Published by EDP Sciences