Radio eclipse of the slowest spinning Galactic-field spider pulsar PSR J1932+2121 and its X-ray emission prospect

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Table 2.

Fitting parameters.

Parameter	PSR J1932+2121
Inclination angle of observer, i_o (°)	$88 . 55_{- 3.90}^{+ 2.12}$ $Mathematical equation: $ 88.55^{+2.12}_{-3.90} $$
True anomaly of observer, ϕ_o (°)	$92 . 76_{- 0.13}^{+ 0.09}$ $Mathematical equation: $ 92.76^{+0.09}_{-0.13} $$
Mass-loss rate, log₁₀ Ṁ_C (M_⊙ yr⁻¹)	$- 12 . 46_{- 0.02}^{+ 0.05}$ $Mathematical equation: $ -12.46^{+0.05}_{-0.02} $$
Wind velocity, v_w (10⁸ cm s⁻¹)	$0 . 34_{- 0.03}^{+ 0.06}$ $Mathematical equation: $ 0.34^{+0.06}_{-0.03} $$
Magnetic field perpendicular to LOS, B_m sin θ (G)	$2 . 17_{- 0.26}^{+ 0.43}$ $Mathematical equation: $ 2.17^{+0.43}_{-0.26} $$
Effective nonthermal fraction, f (10⁻²)	$1 . 34_{- 0.43}^{+ 0.41}$ $Mathematical equation: $ 1.34^{+0.41}_{-0.43} $$

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