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Temperature Variations on the Surface of the Si-star CU Virginis

Published online by Cambridge University Press:  12 April 2016

T.A. Ryabchikova
T.A. Ryabchikova*
Affiliation:
Astronomical Council of the USSR Academy of Sciences, Moscow, USSR

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
Information
International Astronomical Union Colloquium , Volume 130: The Sun and Cool Stars: activity, magnetism, dynamos , 1991 , pp. 350 - 352
Copyright
Copyright © Springer-Verlag 1991

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