Pulsar PRS 0656 + 14 - Period and spindown

Details Pulsar PRS 0656 + 14 - Period and spindown Pulsar PRS 0656 + 14 - Period and spindown

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...161..303d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 161, no. 2, June 1986, p. 303, 304.

Astronomy and Astrophysics

Astrophysics

10

Periodic Variations, Pulsars, Least Squares Method, Secular Variations, Spin

Scientific paper

Observations from various sources are used to explain the larger-than-expected period noted for pulsar 0656 + 14 on July 7, 1984 (Ashworth and Lyne, 1981). No indication of orbital motion was found, and most of the observations are consistent with a simple secular spindown. The derived period derivative of (54.3 + or - 1.3) x 10 to the -15th at epoch 2444300 is far greater than the previously reported value.

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