Gravitational radiation from a star that is contracting into a disk

Details Gravitational radiation from a star that is contracting into a disk Gravitational radiation from a star that is contracting into a disk

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975azh....52..657n&link_type=abstract

Astronomicheskii Zhurnal, vol. 52, May-June 1975, p. 657-659. In Russian.

Astronomy and Astrophysics

Astronomy

4

Astronomical Models, Gravitational Collapse, Gravitational Waves, Stellar Evolution, Stellar Radiation, Energy Transfer, Free Fall, Stellar Gravitation, Stellar Rotation

Scientific paper

Emission of gravitational radiation from a star that is contracting into a disk is analyzed in the framework of the Thuan-Ostriker (1974) model of a collapsing uniformly rotating spheroid. It is shown that during stellar collapse to a disk, the major portion of energy will be radiated in a burst when the contraction of matter abruptly halts at the moment of flattening. Corresponding formulas are given.

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