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- W2078164002 abstract "Binary pulsar systems are superb probes of stellar and binary evolution and the physics of extreme environments. In a survey with the Arecibo telescope, we have found PSR J1903+0327, a radio pulsar with a rotational period of 2.15 milliseconds in a highly eccentric (e = 0.44) 95-day orbit around a solar mass (M(middle dot in circle)) companion. Infrared observations identify a possible main-sequence companion star. Conventional binary stellar evolution models predict neither large orbital eccentricities nor main-sequence companions around millisecond pulsars. Alternative formation scenarios involve recycling a neutron star in a globular cluster, then ejecting it into the Galactic disk, or membership in a hierarchical triple system. A relativistic analysis of timing observations of the pulsar finds its mass to be 1.74 +/- 0.04 M solar symbol, an unusually high value." @default.
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- W2078164002 date "2008-06-06" @default.
- W2078164002 modified "2023-10-10" @default.
- W2078164002 title "An Eccentric Binary Millisecond Pulsar in the Galactic Plane" @default.
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- W2078164002 doi "https://doi.org/10.1126/science.1157580" @default.
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