X-ray Emission from YSOs, Protostellar Jets, and Accretion Eruptive Variables

Details X-ray Emission from YSOs, Protostellar Jets, and Accretion Eruptive Variables X-ray Emission from YSOs, Protostellar Jets, and Accretion Eruptive Variables

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop..173s&link_type=abstract

XMM-Newton Proposal ID #06740601

Physics

Stars, White Dwarfs, Solar System, Field1

Scientific paper

Imaging in X-rays has become an extremely useful tool to identify YSOs residing in star forming regions. X-ray emission is also being measured in eruptive young stars, the FUOr-EXOr type stars, and in protostellar jets. Recent deep near-IR imaging of the North American and Pelican nebulae in JHKs and narrowband emission lines of H2 and [FeII] have revealed one of the most active, richest star forming regions in the Galaxy. Within a single EPIC FOV lies dozens of resolved outflows, jets, clusters of YSOs, and even eruptive FUOR-EXOr stars currently undergoing outbursts. I propose to obtain XMM-Newton imaging of three regions rich in all three types of objects to render x-ray detections to assist with confirming the YSOs, and to measure the x-ray flux of the eruptive stars and shocked outflows.

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