Astronomy Letters

, Volume 28, Issue 3, pp 143–149 | Cite as

Broadband gravitational-wave pulses from binary neutron stars in eccentric orbits

  • A. V. Gusev
  • V. B. Ignatiev
  • A. G. Kuranov
  • K. A. Postnov
  • M. E. Prokhorov


The gravitational-wave radiation from binary stars in elliptical orbits peaks at times close to the periastron passage. For a stationary distribution of binary neutron stars in the Galaxy, there are several systems with large orbital eccentricities and periods in the range from several tens of minutes to several days from which gravitational-wave radiation at periastron will be observed as a broad pulse in the frequency range 1–100 mHz. The LISA space interferometer will be able to record pulsed signals from these systems at a signal-to-noise ratio \(S/N > 5\sqrt 5\) in the frequency range ∼10−3–10−1 Hz. Algorithms for detecting such signals are discussed.


Radiation Neutron Star Stationary Distribution Pulse Signal Elliptical Orbit 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© MAIK "Nauka/Interperiodica" 2002

Authors and Affiliations

  • A. V. Gusev
    • 1
  • V. B. Ignatiev
    • 2
  • A. G. Kuranov
    • 1
  • K. A. Postnov
    • 1
    • 3
  • M. E. Prokhorov
    • 1
  1. 1.Sternberg Astronomical InstituteMoscowRussia
  2. 2.Moscow State UniversityVorob’evy gory, MoscowRussia
  3. 3.Max-Planck-Institut für AstrophysikGarching bei MÖnchenGermany

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