Computer Science
Scientific paper
Sep 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cxo..prop.1379f&link_type=abstract
Chandra Proposal ID #05200123
Computer Science
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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