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THE BM Ori system. IV. A new component of the system

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Abstract

Cross correlations between observed and synthetic spectra are used to discover yet another satellite of BM Ori with the following characteristics: effective temperature Teff = 4000 K, radius R = 16R⊙, mass M = 1.8M⊙, spectral type K7 III, absolute bolometric stellar magnitude Mb = + 4m·0, axial rotation velocity V sini = 85 km/s, and relative luminosity 0.005 near the V band.

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Authors and Affiliations

  1. Institute of Space Research, Russian Academy of Sciences, Russia

    É. A. Vitrichenko

  2. Special Astrophysical Observatory, Russian Academy of Sciences, Russia

    V. G. Klochkova

  3. Taurian National University, Crimea, Ukraine

    V. V. Tsymbal

Authors
  1. É. A. Vitrichenko
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  2. V. G. Klochkova
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  3. V. V. Tsymbal
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Translated from Astrofizika, Vol. 49, No. 1, pp. 111–120 (February 2006).

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Vitrichenko, É.A., Klochkova, V.G. & Tsymbal, V.V. THE BM Ori system. IV. A new component of the system. Astrophysics 49, 96–104 (2006). https://doi.org/10.1007/s10511-006-0011-5

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  • DOI: https://doi.org/10.1007/s10511-006-0011-5

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