Wobble radiation from pulsars.

Details Wobble radiation from pulsars. Wobble radiation from pulsars.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cha%26a..13..345g&link_type=abstract

Chin. Astron. Astrophys., Vol. 13, No. 4, p. 345 - 349

Astronomy and Astrophysics

Astrophysics

Pulsars: Gravitational Radiation

Scientific paper

The authors derive the post-Newtonian multipole 'wobble' radiation formula taking into account self-gravity, internal stress and internal motion by means of the general multipole-moment formula of Epstein and Wagoner. Applying their formula to the Crab and Vela pulsars, the authors find the power to be 1.8 times that of the quadrupole radiation. The excess comes mainly from the self-gravity of the source. Thus, it is important to include the self-gravity and to use the mutipole-moment formula when considering gravitational radiation from astrophysical sources.

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