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The short period magnetic variable HD 133029

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Abstract

It is shown that the magnetic measurements of HD 133029 exhibit a correlation of magnetic intensity with exposure length. Due to this effect a re-examination of the star's period was undertaken, resulting in a new period of 0.168 days. The significance of such a short period is discussed. It is argued that this short variation cannot be due to an oblique rotator.

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Authors and Affiliations

  1. Department of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, Israel

    Raphael Steinitz & Diane M. Pyper

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  1. Raphael Steinitz
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  2. Diane M. Pyper
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Steinitz, R., Pyper, D.M. The short period magnetic variable HD 133029. Astrophys Space Sci 11, 322–329 (1971). https://doi.org/10.1007/BF00661362

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  • DOI: https://doi.org/10.1007/BF00661362

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