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