Abstract
Radio monitoring of RS CVn systems is being carried out with the Noto VLBI antenna. Preliminary results on flare activity on HR 1099 are here presented. During one of these radio bursts we made VLBI observations which provide information about the source angular dimension and brightness temperature.
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© 1993 Kluwer Academic Publishers
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Trigilio, C., Umana, G., Catalano, S., Rodonò, M., Frasca, A. (1993). Single-Dish Monitoring of RS CVn Binary Systems. In: Linsky, J.F., Serio, S. (eds) Physics of Solar and Stellar Coronae: G.S. Vaiana Memorial Symposium. Astrophysics and Space Science Library, vol 183. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1964-1_57
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DOI: https://doi.org/10.1007/978-94-011-1964-1_57
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-2346-4
Online ISBN: 978-94-011-1964-1
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