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Summary

An HSO survey of nearby SFR can attack two of the most challenging problems in Star Formation: the origin of the stellar IMF and the evolution of protoplanetary disks
The sensitivity, angular resolution and mapping speed of HSO will allow to map large areas of nearby Star Forming Complexes in a short time
The preparation of the observing program and the required simulations are in progress

Summary

An HSO survey of nearby SFR can attack two of the most challenging problems in Star Formation: the origin of the stellar IMF and the evolution of protoplanetary disks

The sensitivity, angular resolution and mapping speed of HSO will allow to map large areas of nearby Star Forming Complexes in a short time

The preparation of the observing program and the required simulations are in progress