2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/36446This note describes fitting formulae for the gravitational waveforms generated by a rapidly rotating neutron star (e.g., newly-formed in the core collapse of a supernova) as it evolves from an initial axisymmetric configuration toward a triaxial ellipsoid.TeX, 3 pagesGeneral Relativity and Quantum Cosmologytext