Hostname: page-component-745bb68f8f-b95js Total loading time: 0 Render date: 2025-01-08T21:14:01.631Z Has data issue: false hasContentIssue false
  • English
  • Français

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
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Einstein, A. 1916, Annalender Physik, 354, 769CrossRefGoogle Scholar
Kalomeni, B.: 2010, IAU Symposium, 262, 362.Google Scholar
Köse, O. & Yakut, K.: 2012, in preparation.Google Scholar
Nelemans, G., Yungelson, L. R. & Portegies Zwart, S. F.: 2001, A&A, 375, 890.Google Scholar
Paczynski, B. & Sienkiewicz, R.: 1981, ApJ, 248, L27.CrossRefGoogle Scholar
Phinney, E. S.: 1991, ApJ, 380, L17.CrossRefGoogle Scholar
Verbunt, F. & Zwaan, C.: 1981, A&A, 100, L7.Google Scholar
Yakut, K., Kalomeni, B., & Tout, C. A.: 2008, ArXiv e-prints, arXiv:0811.0455.Google Scholar