Fig. 7.
Gravitational wave amplitude from Eq. (1a) and from Eq. (5b) as a function of the magnetic field at the surface (pole), Bs, (left), and the gravitational mass (right) for the NL3ωρ model. We assumed a family of stars located at a distance of 1 kpc and spinning with a frequency of 1 Hz. The black dots correspond to the two-solar-mass star configurations.
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