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