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We should note that the neutrino damping of nonradial pulsations discussed by D. Kazanas and D. N. Schramm, Astrophys. J. 214, 819 (1977), is not relevant here. The nonaxisymmetric configuration is a lowest-energy (equilibrium) state of the core and is not associated with pulsations.^^The arguments presented earlier with regard to magnetic fields apply even more strongly here. If neutron-star fields are any indication, there simply is not enough time for sufficient winding of the field lines. ^^B. D. Miller, Astrophys. J. 187, 609 (1974); M. N. Fedorov and V. P. Tsvetkov, Zh. Eksp. Teor. Fiz. 65^, 1289) [Sov. Phys. JETP 38, 641 (1974] . ^^Descriptions of representative experiments are given by J. Weber, Phys. Rev. Lett. 22, 1320Lett. 22, (1969;