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Binary Systems As Gravitational Wave Sources

Published online by Cambridge University Press:  23 April 2012

O. Köse  and
K. Yakut
O. Köse
Affiliation:
Department of Astronomy and Space Sciences, University of Ege, 35100, İzmir, Turkey
K. Yakut
Affiliation:
Department of Astronomy and Space Sciences, University of Ege, 35100, İzmir, Turkey Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
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Abstract

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Binary systems with compact components and some newly discovered systems with relatively short orbital periods are studied as gravitational-wave sources. The gravitational wave amplitudes of these systems have been compared with the limit of gravitational wave interferometers (e.g. LISA, LIGO, and VIRGO).

Keywords

gravitationgravitational wavesstars: binaries: close
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S282: From Interacting Binaries to Exoplanets: Essential Modeling Tools , July 2011 , pp. 468 - 469
Copyright
Copyright © International Astronomical Union 2012

References

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