PSR J1744-3922: Hint of a New Binary Pulsar Class
Standard binary evolution models of pulsars in very circular orbits can explain systems with lighter companions and weaker magnetic fields: they are descended from long-lived Low Mass X-ray Binaries with Roche-lobe overflow. By contrast, those having more massive companions and larger magnetic fields are descendants of Intermediate Mass systems
Breton, R. P. et al.
Fecha de publicación:
2
2008