A six year timing solution for PSR B1951 + 32

Details A six year timing solution for PSR B1951 + 32 A six year timing solution for PSR B1951 + 32

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aj....108..175f&link_type=abstract

The Astronomical Journal, vol. 108, no. 1, p. 175-178

Astronomy and Astrophysics

Astronomy

13

Pulsars, Radio Astronomy, Supernova Remnants, Time Measurement, Stellar Luminosity, Stellar Radiation, Very Large Array (Vla)

Scientific paper

Six years of pulse time-of-arrival measurements have been collected from observations of the young, fast pulsar PSR B1951 + 32 in the CTB 80 supernova remnant using the Jodrell Bank and Arecibo radio telescopes. The combined data allow for the determination of a phase connected solution between 1987 August 21 and 1993 September 21. This solution provides an accurate rotational ephemeris for high energy x-ray and gamma-ray observations of this source made during the six years of radio timing observations to an accuracy of better than one tenth of a pulse period (4 ms). The pulsar has an activity parameter comparable with the value seen in the Crab pulsar.

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