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The Carina Nebula is an ideal site to study violent high-mass star
formation and the effects of massive star feedback,
via stellar winds, ionizing radiation, and expanding superbubbles,
on their surroundings.
I will present first results of an ongoing comprehensive
multi-wavelength (X-ray to & sub-mm) observational survey
of this important region, that will allow to
reveal the full stellar populations, study their ages, mass functions,
and disk properties and to probe the morphology, fragmentation,
kinematics, and chemistry of the molecular clouds
throughout the complex.
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