Young Stars in the Orion Trapezium Cluster

Details Young Stars in the Orion Trapezium Cluster Young Stars in the Orion Trapezium Cluster

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..217g&link_type=abstract

Chandra Proposal ID #01200039

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Chandra Proposal Id #01200039

Scientific paper

The Orion Trapezium cluster is the richest and densent cluster of pre-main sequence stars in the solar neighborhood, and the nearest region of high-mass star forming region. It is a superb laboratory for study of X-ray emission from protostars, classical and weak-lined T Tauri stars. The proposed observation should detect hundreds of stars, dozens of powerful magnetically-induced flares. X-ray emission from embedded protostars and massive OB stars will also be studied. The relationaships between X-ray emission and other stellar properties, and the influence of magnetic activity on star and planet formation, will be investigated.

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