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

Copyright ESO 2003
Published by EDP Sciences