Abstract
We are carrying out an infrared monitoring program of RS CVn systems devoting special attention to the short-period group. The observations are made with the 1.5 m C.S. telescope at the Observatorio de Izaña (Tenerife, Canary Islands) using an infrared single-channel photometer with an InSB detector cooled with liquid nitrogen. The system is compatible with Johnson (Arribas and Martinez-Roger, 1986).
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Arévalo, M.J., Lázaro, C. (1990). Infrared photometry of RS CVn short-period systems. In: İbanoğlu, C. (eds) Active Close Binaries. NATO ASI Series, vol 319. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0679-2_37
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DOI: https://doi.org/10.1007/978-94-009-0679-2_37
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