Abstract
RZ LMi is the object with a strong UV excess. Depending on the brightness of the variable, emission or absorption hydrogene lines are observed.
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© 1995 Springer Science+Business Media Dordrecht
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Pikalova, O.D., Shugarov, S.Y. (1995). The Photometric Investigation of RZ LMi. In: Bianchini, A., Valle, M.D., Orio, M. (eds) Cataclysmic Variables. Astrophysics and Space Science Library, vol 205. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0335-0_55
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DOI: https://doi.org/10.1007/978-94-011-0335-0_55
Publisher Name: Springer, Dordrecht
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