Table 2.
Comparison between the barotropic models described in Section 5.4.
| Location | α | HWHM [HP] | ΔPa [s] | Δnglitch | Pglitch [min] | Φ(rglitch) |
|---|---|---|---|---|---|---|
| Boundary | ∞ | 0 | 258.67 | ∞ | ∞ | 0 |
| Boundary | 103 | 0.0012 | 255.7 | 84.6 | 360.7 | 0.0118 |
| Boundary | 102 | 0.012 | 250.27 | 27.14 | 113.2 | 0.037 |
| Boundary | 10 | 0.16 | 236.98 | 0 | 0 | – |
| Radiative core | ∞ | 0 | 265.3 | 11.69 | 51.6 | 0.086 |
| Radiative core | 50 | 0.03 | 250.92 | 8.50 | 35.5 | 0.117 |
| Radiative core | 10 | 0.17 | 246.56 | 0 | 0 | – |
Notes. The first column presents the location of a density discontinuity, which may occur at the boundary between the convective core and the radiative core or situated within the radiative core itself. The second and third columns refer to the width of the bell-shaped structures incorporated in the models. The fourth column presents the asymptotic period spacing, while the subsequent columns indicate the periodicity of the glitches that have been observed (if any) along with their inferred locations.
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