On the proper motion of the binary pulsar PSR 1913 + 16

Details On the proper motion of the binary pulsar PSR 1913 + 16 On the proper motion of the binary pulsar PSR 1913 + 16

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...310..719m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 310, Nov. 15, 1986, p. 719-722.

Astronomy and Astrophysics

Astrophysics

Binary Stars, Pulsars, Stellar Motions, Relativity, Stellar Orbits

Scientific paper

The inferences that may be drawn from the 14 observed values of the periastron passage times of the binary pulsar PSR 1913 + 16, obtained during a period of observations of about 6 yr by Taylor and Weisberg (1982), are presented. The timing formula of an orbiting pulsar is briefly discussed, and the formula is modified slightly for the case where the interval of observations is many times the orbital period. This result is applied to the binary system under consideration, obtaining the result that the projection of the center-of-mass velocity over the orbital plane cannot exceed 15 km/s.

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