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The Highly Relativistic Binary Pulsar PSR J0737-3039A: Discovery and Implications
M. Burgay, N. D'Amico, A. Possenti +10
PSR J0737-3039A is a millisecond pulsar with a spin period of 22.7 ms included in a double-neutron star system with an orbital period of 2.4 hrs. Its companion has also been detect…
The double pulsar -- A new testbed for relativistic gravity
M. Kramer, A. G. Lyne, M. Burgay +9
The first ever double pulsar, discovered by our team a few months ago, consists of two pulsars, one with period of 22 ms and the other with a period of 2.7 s. This binary system wi…
Two clocks in the PSR J0737--3039 binary system and their implications for the system's origin and evolution
D. R. Lorimer, M. Burgay, P. C. C. Freire +8
As discussed elsewhere in these proceedings, the double pulsar system is a magnificent laboratory for gravitational physics and for studying pulsar magnetospheres. Here we consider…
New Binary and Millisecond Pulsars from Arecibo Drift-Scan Searches
M. A. McLaughlin, D. R. Lorimer, D. J. Champion +6
We discuss four recycled pulsars found in Arecibo drift-scan searches. PSR J1944+0907 has a spin period of 5.2 ms and is isolated. The 5.8-ms pulsar J1453+19 may have a low-mass co…