Limits on pulsar planetary systems from the Jodrell Bank timimg database

Details Limits on pulsar planetary systems from the Jodrell Bank timimg database Limits on pulsar planetary systems from the Jodrell Bank timimg database

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aspc...36...19b&link_type=abstract

In: Planets around pulsars; Proceedings of the Conference, California Inst. of Technology, Pasadena, Apr. 30-May 1, 1992 (A93-36

Physics

14

Extrasolar Planets, Planetary Systems, Pulsars, Planetary Mass, Stellar Orbits, Time Measurement

Scientific paper

The Jodrell Bank timing database is used to verify the existence of a sinusoidal feature with a period of about 1,100 days in the pulse timing residuals of the pulsar PSR 0329+54, claimed by Demianski and Proszynski (1979). Data obtained indicate that there are no obvious signatures of planetary systems. The pulsar PSR 1828-11 contains a large amount of timing noise, and has postfit residuals that can be modelled quite successfully by two sinusoids, but only after the removal of a significant period second derivative.

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