Here we describe optical and radio observations which rule out most of the scenarios proposed to explain formation of this system. Radio timing measurements of three post-Keplerian effects yield the ...
We have detected a pulsar with a pulsation period that varies systematically between 0.058967 and 0.059045 sec over a cycle of 0.3230 d. Approximately 200 independent observations over 5-minute ...
the secular motion of the pulsar or binary system, interstellar, Solar system and ionospheric dispersion, observatory motion (including Earth rotation, precession, nutation, polar motion and orbital ...
Radio pulsars are rapidly rotating, highly magnetized neutron stars. This comprehensive book brings together key observational techniques, background information and a review of the latest results, ...
Abstract: Each of the two pulsars in the double pulsar PSR J0737-3039A/B system exhibits not only the pulses emanating from it ... (the other pulsar), and is shown to be entirely analogous to the ...