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Application of a new non-linear least squares velocity curve analysis technique for spectroscopic binary stars

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Abstract

Using measured radial velocity data of nine double lined spectroscopic binary systems NSV 223, AB And, V2082 Cyg, HS Her, V918 Her, BV Dra, BW Dra, V2357 Oph, and YZ Cas, we find corresponding orbital and spectroscopic elements via the method introduced by Karami and Mohebi (Chin. J. Astron. Astrophys. 7:558, 2007a) and Karami and Teimoorinia (Astrophys. Space Sci. 311:435, 2007). Our numerical results are in good agreement with those obtained by others using more traditional methods.

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Authors and Affiliations

  1. Department of Physics, University of Kurdistan, Pasdaran St., P.O. Box 66177-15175, Sanandaj, Iran

    K. Karami, R. Mohebi & M. M. Soltanzadeh

  2. Research Institute for Astronomy & Astrophysics of Maragha (RIAAM), P.O. Box 55134-441, Maragha, Iran

    K. Karami

  3. Institute for Advanced Studies in Basic Sciences (IASBS), Gava Zang, P.O. Box 45195-1159, Zanjan, Iran

    K. Karami

Authors
  1. K. Karami
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  2. R. Mohebi
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  3. M. M. Soltanzadeh
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Correspondence to K. Karami.

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Karami, K., Mohebi, R. & Soltanzadeh, M.M. Application of a new non-linear least squares velocity curve analysis technique for spectroscopic binary stars. Astrophys Space Sci 318, 69–71 (2008). https://doi.org/10.1007/s10509-008-9905-5

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  • DOI: https://doi.org/10.1007/s10509-008-9905-5

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