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The IMF of the Orion Nebula Cluster Across the H-burning Limit

The IMF of the Orion Nebula Cluster Across the H-burning Limit. Nicola Da Rio HST Orion Treasury Science Meeting STScI, Baltimore, September 12 th 13 th 2011. Motivation. In order to derive the properties of PMS stars in Orion we need individual spectral types.

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