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New photoelectric observations and light curve analysis of 44i bootis

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Abstract

The eclipsing binary 44i Boo was observed photoelectrically using the 40 cm Cassegrain telescope at the Al-Battani Observatory.

The light curves were analysed using Fourier techniques of light changes in the frequency-domain, and new geometrical and physical elements have been obtained.

A new active period to be started in 1986 has been observed.

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Authors and Affiliations

  1. Astronomical Research Unit, Scientific Research Council, Al-Jadiriah, Baghdad, Iraq

    Hamid M. K. Al-Naimiy, Hasan A. Fleyeh, Aasem O. Al-Sikab & Jinan M. Al-Razzaz

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  1. Hamid M. K. Al-Naimiy
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  2. Hasan A. Fleyeh
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  3. Aasem O. Al-Sikab
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  4. Jinan M. Al-Razzaz
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Al-Naimiy, H.M.K., Fleyeh, H.A., Al-Sikab, A.O. et al. New photoelectric observations and light curve analysis of 44i bootis. Astrophys Space Sci 151, 135–147 (1989). https://doi.org/10.1007/BF00643635

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  • DOI: https://doi.org/10.1007/BF00643635

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