The HETG Orion Legacy Project: PMS Stellar Studies of the Orion Trapezium Cluster

Details The HETG Orion Legacy Project: PMS Stellar Studies of the Orion Trapezium Cluster The HETG Orion Legacy Project: PMS Stellar Studies of the Orion Trapezium Cluster

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2322c&link_type=abstract

Chandra Proposal ID #09200065

Computer Science

Chandra Proposal Id #09200065

Scientific paper

The Trapezium Cluster at the center of the Orion Nebula Cluster (ONC) is one of the youngest and closest (440 pc) star-forming regions. Many of the properties we know today are derived from X-ray signatures. Here we study highly resolved X-ray spectra of a large ensemble of very young and chemically similar PMS stars in terms of their magnetic and accretion properties. This is the forth of several installments of our Orion HETG Legacy Program, which already amounts to 430 ks by the end of AO8. There are two installments of 75 ks in AO9. This is the second installment which will lead to the final exposure of the project of 580 ks. On completion we expect about a dozen of well exposed HETG PMS star spectra and HETG Trapezium spectra of supreme quality. .

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