High-energy pulses and phase-resolved spectra by inverse Compton emission in the pulsar striped wind - Application to Geminga

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Table 1:

Properties of the Geminga pulsar assuming R_*=10 km. Period, distance and magnetic field strength are taken from Taylor et al. (1993).
Pulsar	P (ms)	d (kpc)	$\log(B)$ (T)	$B_{\rm L}$ (T)	$R_{\rm L}$ (km)	$\zeta$ (degree)	$\chi$ (degree)
Geminga	237.09	0.15	8.21	0.112	11 312.4	90	60

Source LaTeX | All tables | In the text

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