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Article Contents
1 Introduction
2 Measuring deviations from Keplerian rotation in spatially unresolved protostellar disks
3 Basic parameters for a model suggested by the SED of FU Ori
4 Optical-NIR line profiles
5 Probing the outer disk rotation with H2 line profiles
6 Sub-mm CO line profiles
7 Conclusions

List of tables
List of figures

Copyright ESO 2003
Published by EDP Sciences