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Temperature Variations on the Surface of the Si-star CU Virginis
Published online by Cambridge University Press: 12 April 2016
Abstract
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A hot region with an increase of effective temperature of 700 K was found on the surface of Si-star CU Vir, based on the analysis of the available photometric and spectroscopic observations. This hot region is located near the phase of negative magnetic extremum and can explain both hydrogen line and infrared light variations.
- Type
- Part IV Stellar activity
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- Copyright © Springer-Verlag 1991
References
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