RX And: An intermediate between Z Cam and VY Scl stars

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Abstract

We present the AAVSO long term visual light curve of RX And. The system has been classified as a Z Cam-type dwarf nova, showing alternating standstills and dwarf nova outbursts. Our data reveal that RX And has also characteristics of a VY Scl star, remaining for extended periods in a low state ∼3.5 mag fainter than the standstill with no detectable outbursts. We discuss this result in the context of mass transfer variations in CVs and the still poorly understood VY Scl phenomenon.

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Schreiber, M. R., Gänsicke, B. T., & Mattei, J. A. (2002). RX And: An intermediate between Z Cam and VY Scl stars. Astronomy and Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361:20020122

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