Abstract
Spectrophotometric observations of the RS CVn binary UX Arietis have been presented. The comparison of the observed fluxes with model atmospheres indicates that during the four phases observed, the temperature does not vary significantly. However, brightness variation of 0m.23 are thought to be due to change in the surface emitting regions.
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Joshi, S.C., Srivastava, R.K. & Srivastava, J.B. Spectrophotometric observations of UX arietis. Astrophys Space Sci 183, 11–15 (1991). https://doi.org/10.1007/BF00643014
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DOI: https://doi.org/10.1007/BF00643014