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1 Introduction
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2 Examination of claimed observational evidence for enhanced mass
transfer during outburst
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3 Theoretical aspects for enhanced mass transfer from irradiated
secondary stars
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4 Smak's (1996) criticism and a new picture of the TTI model
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5 The overall picture of the 2001 outburst of WZ Sge
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6 Conclusion
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Appendix A: Comments on Kato's (2002) model for early humps
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References
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