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Optical and other high energy emission


tex2html_wrap_inline3922   Mostly the very youngest pulsars
tex2html_wrap_inline3922   Just 3 pulsars detected at Optical Wavelengths
tex2html_wrap_inline3922   Crab, Vela, B0540-69
tex2html_wrap_inline3922   X-ray - 27 detected, 13 pulsed
tex2html_wrap_inline3922   Gamma ray - 6 detected all pulsed
tex2html_wrap_inline3922   Radio emission tex2html_wrap_inline4114 of spin down energy
tex2html_wrap_inline3922   Opt,X, tex2html_wrap_inline2816 account for few %
tex2html_wrap_inline3922   Learn much more about magnetosphere etc
tex2html_wrap_inline3922   Mostly double peaked profiles from wide cones
tex2html_wrap_inline3922   Need radio ephemeris
tex2html_wrap_inline3922   18000 pulse periods elapse between each EGRET photon detected from the Crab pulsar

Jon Bell
Thu Dec 19 15:15:11 GMT 1996