Planetary Companions of Pulsars

Details Planetary Companions of Pulsars Planetary Companions of Pulsars

May 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970natur.226..730h&link_type=abstract

Nature, Volume 226, Issue 5247, pp. 730-731 (1970).

Computer Science

12

Scientific paper

THE recent observation of a ``quasi-sinusoidal'' period variation in the pulsar NP 0532 has been attributed to perturbations produced by a planetary companion with an orbital period of about three months and a minimum mass of 1.0 M⊕ assuming the mass of the pulsar to be 1 Msolar (ref. 1). It is therefore desirable to investigate the orbit of a planet after a supernova explosion of the central star, and the effect of the new orbit on the observed period of the pulsar.

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