next up previous
Next: Strong v Weak tests Up: Binary Neutron Stars Previous: Orbital Velocities

The magnetic fields of the millisecond pulsars

 

tex2html_wrap_inline3922   tex2html_wrap_inline16180 lower than normal pulsars
tex2html_wrap_inline3922   Why/how are they lower
tex2html_wrap_inline3922   Did the field decay prior to, or during accretion
tex2html_wrap_inline3922   Models for both possibilities exist
tex2html_wrap_inline3922   Both have many shortcomings



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