Self-energy losses in the binary pulsar PSR 1913 + 16

Details Self-energy losses in the binary pulsar PSR 1913 + 16 Self-energy losses in the binary pulsar PSR 1913 + 16

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...174..355s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 174, no. 1-2, March 1987, p. 355, 356.

Astronomy and Astrophysics

Astrophysics

3

Binary Stars, Pulsars, Stellar Orbits, Energy Dissipation, Stellar Gravitation, Stellar Radiation

Scientific paper

The possibility of observationally checking the orbital-period shortening and mass-energy loss of the pulsar PSR 1913 + 16 is examined. The procedures for checking the mass-energy loss are described. It is determined that an improvement in the accuracy of the observed values of the orbital period's rate of change and the associated uncertainity allow for the distinction between the orbital-period shortening caused by self-energy losses and that caused by gravitational-radiation losses.

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