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A runaway binary star escaping from the Θ1 ori system

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A runaway binary star escaping in runaway from the multiple system Θ1 Ori C is studied. The radial velocities of both components are measured and radial velocity curves are constructed and solved for them. The physical parameters and chemical compositions of the stars are determined.

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Authors and Affiliations

  1. Institute of Space Studies, Russian Academy of Sciences, Moscow, Russia

    E. Vitrichenko

  2. Taurian National University, Simferopol, Ukraine

    V. Tsymbal

  3. Special Astrophysical Observatory, Russian Academy of Sciences, Moscow, Russia

    L. Bychkova & V. Bychkov

Authors
  1. E. Vitrichenko
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  2. V. Tsymbal
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  3. L. Bychkova
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  4. V. Bychkov
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Corresponding author

Correspondence to E. Vitrichenko.

Additional information

Translated from Astrofizika, Vol. 54, No. 1, pp. 81–88 (February 2011).

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Vitrichenko, E., Tsymbal, V., Bychkova, L. et al. A runaway binary star escaping from the Θ1 ori system. Astrophysics 54, 68–74 (2011). https://doi.org/10.1007/s10511-011-9158-9

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  • DOI: https://doi.org/10.1007/s10511-011-9158-9

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