New Binary and Millisecond Pulsars from Arecibo Drift-Scan Searches

Details New Binary and Millisecond Pulsars from Arecibo Drift-Scan Searches New Binary and Millisecond Pulsars from Arecibo Drift-Scan Searches

2004-04-08

arxiv.org/abs/astro-ph/0404181v1

Astronomy and Astrophysics

Astrophysics

6 pages, 3 figures, to appear in proceedings of Aspen Center for Physics Conference on ``Binary Radio Pulsars'' Eds. F. Rasio

Scientific paper

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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