Radio Observations of the Carina Nebula: A study of the Proplyds in extreme environments

Computer Science

Scientific paper

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Star Formation, Atca

Scientific paper

We aim to image at cm wavelengths with a high angular resolution (~ 2'') and with great sensitivity the Carina Nebula. These observations will characterize the nature and evolution of the material around Sun-like stars in an environment that may well be an analog to our own birth-site. We will measure the mass loss rates directly from these Carina objects and compare them with those in Orion, in order to understand how the extreme environments play a role in the evolution of these objects.

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