Binary pulsar PSR 1913 + 16 - Model for its origin

Details Binary pulsar PSR 1913 + 16 - Model for its origin Binary pulsar PSR 1913 + 16 - Model for its origin

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sci...188..930v&link_type=abstract

Science, vol. 188, May 30, 1975, p. 930-933.

Astronomy and Astrophysics

Astronomy

5

Astronomical Models, Binary Stars, Companion Stars, Pulsars, Stellar Evolution, Dynamic Stability, Gravitational Effects, Neutron Stars, Orbital Elements, Tides

Scientific paper

It is pointed out that the object reported by Taylor and Hulse (1974) is the first pulsar which shows reliable evidence of binary motion. The data concerning the pulsar are sufficiently restrictive to lead to a nearly unique model. The nature of the secondary star is considered along with questions of system evolution and mass transfer. Observational programs are proposed for supplementing the theoretical analysis conducted.

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