nBraje
and Romani, 2002
Þ Can rotation smear out spectral
features?
Bow shock nebula powered by a relativistic
wind of e± generated
by the pulsar spin-down Þ
estimate of the spin down power
dE/dt ~ I W dW/dt ~ 8 x1032 erg/s
Magneto-dipolar breaking (PdP/dt
»10-15B122)
dE/dt ~ 1034 (B12 t6)-2 erg/s
Þ B12 t6 ~ 3
Also: no pulsations
within 4% gave an allowed fraction of sky 2-4%
This
fraction is even smaller with the new upper limit on the pulsed fraction of
1%