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Radial velocity study of the Be star ξ Tau (HR 1910)

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Abstract

Extensive radial velocity investigation has been presented in this paper for the bright Be star HR 1910, based upon thirty-three spectrograms. The analysis of these radial velocity measurments has demonstrated clearly the binary nature of the star and new orbital elements were determined. A brief discussion of the previous work on this system appears in the relevant sections.

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  1. Astronomy and Space Research Centre, Council for Scientific Research, Jadiriyah, Baghdad, Iraq

    M. M. Jarad

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  1. M. M. Jarad
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Jarad, M.M. Radial velocity study of the Be star ξ Tau (HR 1910). Astrophys Space Sci 139, 83–91 (1987). https://doi.org/10.1007/BF00643814

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  • DOI: https://doi.org/10.1007/BF00643814

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