An approximate correction to the quadrupole radiation of rotating stars

Details An approximate correction to the quadrupole radiation of rotating stars An approximate correction to the quadrupole radiation of rotating stars

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985acaps...5..105z&link_type=abstract

(Acta Astrophysica Sinica, vol. 5, no. 4, 1985, p. 103-108) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 10, March

Astronomy and Astrophysics

Astrophysics

1

Gravitational Waves, Neutron Stars, Quadrupoles, Stellar Radiation, Stellar Rotation, Correction, Pulsars, Stellar Gravitation, Stellar Models

Scientific paper

The radiative power of normal and neutron stars may be estimated by means of the quadrupole formula; the derivation of this formula, however, neglects the self-gravity, internal stress, and internal motion of a source. On the basis of reasonable assumptions concerning the geometry, rotation, internal motion and self-gravity of rotating stars, an explicit expression is derived for the correction of the quadrupole radiation. This correction is found to be of the order of +60 percent in the case of the pulsar PSR 1937 + 214.

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