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New Binary and Millisecond Pulsars from Arecibo Drift-Scan Searches

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arxiv astro-ph/0404181 v1 pith:X25TKGPY submitted 2004-04-08 astro-ph

M. A. McLaughlin , D. R. Lorimer , D. J. Champion , Z. Arzoumanian , D. C. Backer , J. M. Cordes , A. S. Fruchter , A. N. Lommen & K. M. Xilouris This is my paper
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keywords neutronpulsarbinaryisolatedpulsarsstararecibocompanion
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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 companion. We discuss these pulsars in the context of isolated millisecond pulsar formation and the minimum spin period of neutron stars. The isolated 56-ms pulsar J0609+2130 is possibly the remnant of a disrupted double neutron star binary. The 41-ms pulsar J1829+2456 is in a relativistic orbit. Its companion is most likely another neutron star, making this the eighth known double neutron star binary system.

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