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Binary Star Detection with the GAIA Radial Velocity Spectrometer

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Abstract

Accuracy of the radial velocities and efficiency of the spectroscopic binary detection with the GAIA radial velocity spectrometer (RVS) is evaluated by employing the observed spectra (Cenarro et al., 2001) and simulated GAIA observations. Evaluation is performed in the magnitude range V =10-17 by applying the cross-correlation method.

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References

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Authors and Affiliations

  1. Vilnius University Observatory, Čiurlionio 29, Vilnius, 2009, Lithuania

    Viktoras Deveikis & Julius Sperauskas

  2. Institute of Physics, Goštauto 12, Vilnius, 2600, Lithuania

    Vladas Vansevičius

Authors
  1. Viktoras Deveikis
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  2. Julius Sperauskas
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  3. Vladas Vansevičius
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Deveikis, V., Sperauskas, J. & Vansevičius, V. Binary Star Detection with the GAIA Radial Velocity Spectrometer. Astrophysics and Space Science 280, 133–137 (2002). https://doi.org/10.1023/A:1015535013391

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  • DOI: https://doi.org/10.1023/A:1015535013391

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