The star Θ1 Ori C1, which is the nearest companion of the principal star Θ1 Ori C, is studied using extensive spectral data. Two radial velocity curves are constructed and solved. One of these describes the motion of the principal star and the other, the motion of the companion C1; in both cases the stars rotate about the center of mass of the C + C1 system. The physical parameters (temperature, acceleration of gravity, mass) and chemical composition of the star C1 are determined. A periodicity of 15.4 days associated with the rotation of the principal star is identified in the variations of the radial velocity.
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Translated from Astrofizika, Vol. 55, No. 2, pp. 225-233 (May 2012).
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Vitrichenko, E.A., Bondar, N.I., Bychkova, L. et al. The companion C1 in the Θ1 Ori C system. Astrophysics 55, 199–207 (2012). https://doi.org/10.1007/s10511-012-9228-7
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DOI: https://doi.org/10.1007/s10511-012-9228-7