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Variability of 56 Ari

  • W. Czechowski (a1) and K. Stȩpień (a1)

Abstract

From IUE archival data and visual spectrophotometric observations published by Adelman and Pyper, nearly 20 energy distributions of 56 Ari in different rotational phases were obtained. The light variations in selected spectral bands correlate with spectrum variations. The bolometric flux varies by ˜ 2.5 % over the rotation period.

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Copyright

References

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Adelman, S.J. 1983, Astr. Ap. Suppl., 51, 511.
Adelman, S.J., and Pyper, D.M. 1979, A. J., 84, 1726.
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Stȩpień, K., and Czechowski, W. 1992, in preparation.
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