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Variability of 56 Ari
Published online by Cambridge University Press: 12 April 2016
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.
- Type
- VII. Photometric Variability and Evolutionary Status
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- Copyright © Astronomical Society of the Pacific 1993