Abstract
Symbiotic star AG Peg (HD 207757)? which is still declining from the outburst in the last century, appears to be related to the very slow RT Serpentis type novae: binary stars consisting of a cool M giant and a hot component, which underwent outburst.
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Chochol, D. (1988). Symbiotic Star AG Pegasi — Retrospect and Prospects. In: Mikolajewska, J., Friedjung, M., Kenyon, S.J., Viotti, R. (eds) The Symbiotic Phenomenon. Astrophysics and Space Science Library, vol 145. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2969-2_49
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DOI: https://doi.org/10.1007/978-94-009-2969-2_49
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