Pulsars and neutron stars/Individual pulsars
Appearance
Introduction
[edit | edit source]Individual pulsars
[edit | edit source]PSR J0437-4715
[edit | edit source]PSR J1107-5907
[edit | edit source]Parameter | Value |
---|---|
Right ascension | 11:07:34 |
Declination | -59:07:18 |
Period (s) | 0.25 |
Dispersion measure (cm-3pc) | 40.2 |
Binary | No |
This pulsar has at least two emission states. Usually, it is thought to have three states: strong, weak and "off", but Young et al. (2014) suggested that the "off" state may actually be the bottom end of the pulse-intensity distribution of the weak state. They also showed that the pulsar remains in the strong state for ~200-6000 pulses with apparent nulls of up to a few pulses at a time.