Observational evidence for the two types of dwarf nova outbursts |
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Authors: | J Smak |
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Institution: | (1) Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland |
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Abstract: | Observed characteristics of outbursts of eight dwarf novae are compared with those predicted for the two types of outbursts by the disk instability theory. OY Car, U Gem, VW Hyi, and WX Hyi are identified as Type A, while RX And, SS Cyg, AH Her, and CN Ori — as Type B.Paper presented at the IAU Colloquium No. 93 on Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments , held at Dr. Remeis-Sternwarte Bamberg, F.R.G., 16–19 June, 1986. |
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