Stellar Coronal Spectroscopy of Star-Forming Regions: Orion

Details Stellar Coronal Spectroscopy of Star-Forming Regions: Orion Stellar Coronal Spectroscopy of Star-Forming Regions: Orion

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..212c&link_type=abstract

Chandra Proposal ID #01200028

Physics

Chandra Proposal Id #01200028

Scientific paper

HETGS spectra will reveal a wealth of information on the temperature and density structure of stellar coronae and winds. The Trapezium in Orion contains many hot and cool young stars. HETGS observations of Orion will simultaneously obtain dispersed spectra of the brightest objects (hot stars), and CCD PHA spectra of young cool stars. This observation will also test the abilities of multiple source spectroscopy with HETGS.

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