A comprehensive survey of X-ray emission from the earliest phases of star formation

Computer Science

Scientific paper

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Chandra Proposal Id #05200123

Scientific paper

We propose to conduct a comprehensive survey of X-ray emission from the earliest phases of star formation, in particular of Class O sources. This will be conducted with a deep (100 ks) imaging observation of the Serpens molecular cloud, the best (and nearest) site for the proposed science. Our survey will detect X-ray emission from a significant number of Class 0 and Class I sources, allowing to conclusively establish when does X-ray emission start to become important in the star formation process and to constrain the relevant emission mechanisms.

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