Timing observations of the binary pulsar PSR 1913 + 16

Details Timing observations of the binary pulsar PSR 1913 + 16 Timing observations of the binary pulsar PSR 1913 + 16

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...261l..97b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 261, Oct. 15, 1982, p. L97-L101.

Astronomy and Astrophysics

Astronomy

12

Binary Stars, Gravitational Waves, Orbit Calculation, Pulsars, Stellar Gravitation, Stellar Spectrophotometry, Astrometry, Orbital Elements, Radio Astronomy, Spectrum Analysis, Stellar Rotation

Scientific paper

Observations of the binary pulsar PSR 1913 + 16 made at the Arecibo Observatory are reported. The analysis of these data yields orbital parameters of the binary system which are in agreement with those obtained by J. Taylor (1979) and his collaborators. In particular, the data are consistent with the derived rate of change of the orbital period being attributed to gravitational radiation reaction.

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