Wobble radiation from pulsars

Details Wobble radiation from pulsars Wobble radiation from pulsars

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989acaps...9..239b&link_type=abstract

(Acta Astrophysica Sinica, vol. 9, no. 3, 1989, p. 239-243) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 13, Dec. 1

Astronomy and Astrophysics

Astrophysics

Gravitational Waves, Pulsars, Stellar Gravitation, Stellar Radiation, Astronomical Models, Crab Nebula, Multipolar Fields

Scientific paper

The post-Newtonian multipole 'wobble' radiation formula is derived taking into account self-gravity, internal stress, and internal motion. Applying the formula to the Crab and Vela pulsars, the power is found 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 multipole-moment formula when considering gravitational radiation from astrophysical sources.

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