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Photometric study of BZ Eridani

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Abstract

The 1980–1981U, B, andV observations of the eclipsing binary BZ Eridani have been presented. A new period of BZ Eri comes out to be 0d.6641703. The colour curves of the system show appreciable variations, and are indicative of intrinsic variability. The secondary minimum falls nearly at phase 0.5. Some interesting features are given. The features of BZ Eri are changing. Some light variations are visible around the phase of the secondary minimum. The discussion reveals that BZ Eri is a complicated system.

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Authors and Affiliations

  1. Uttar Pradesh State Observatory, Naini Tal, India

    R. K. Srivastava & Wahab Uddin

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  1. R. K. Srivastava
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  2. Wahab Uddin
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Srivastava, R.K., Uddin, W. Photometric study of BZ Eridani. Astrophys Space Sci 126, 105–118 (1986). https://doi.org/10.1007/BF00644179

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  • DOI: https://doi.org/10.1007/BF00644179

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