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.
CITATION STYLE
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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