Gravitational radiation from dual neutron star elliptical binaries

Details Gravitational radiation from dual neutron star elliptical binaries Gravitational radiation from dual neutron star elliptical binaries

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...381..484h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 381, Nov. 10, 1991, p. 484-489.

Astronomy and Astrophysics

Astrophysics

6

Binary Stars, Gravitational Waves, Neutron Stars, Elliptical Orbits, Galactic Radiation, Milky Way Galaxy

Scientific paper

General expressions are derived for the gravitational radiation incident on earth due to elliptical binary systems in the Galaxy. These results are applied to dual neutron star elliptical binaries. Calculations show that eccentric dual neutron star binaries lead to a moderate increase in gravitational flux density compared with circular systems for frequencies above approximately 0.0001 Hz. Tables of various quantities such as average gravitational luminosity, number of sources per unit bandwidth, energy spectral flux density, and gravitational wave strain density are given.

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