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Article Contents
1 Introduction
2 Self-regulated accretion disks
3 General properties of the spectral energy distribution of active, self-gravitating accretion disks
4 A possible fit to the spectral energy distribution of some FU Orionis systems
5 Difficulties of the self-gravitating scenario in the context of T Tauri stars
6 Conclusions
Appendix A: Fit parameters obtained from the SEDs of some T Tauri systems

Copyright ESO 2001
Published by EDP Sciences