Back to the Abstract


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
References

Copyright ESO 2001
Published by EDP Sciences