An Ultradeep Chandra Study of the Orion Nebula (guest Observer Portion)

Details An Ultradeep Chandra Study of the Orion Nebula (guest Observer Portion) An Ultradeep Chandra Study of the Orion Nebula (guest Observer Portion)

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1135f&link_type=abstract

Chandra Proposal ID #04200331

Physics

Chandra Proposal Id #04200331

Scientific paper

We propose a 850 ks ACIS-I observation of the Orion Nebula spanning 11.5 contiguous days, with GTO Teams providing 150 ks of the time. The Orion Nebula is the best target in the sky for Chandra study of stellar magnetic activity and star formation with extensive multiwavelength support. Science goals include: addressing the mass- and age-dependence of magnetic activity in brown dwarfs; uncovering the low-mass members of the deeply embedded clusters; elucidating the absence of an activity-rotation relation in pre-main sequence stars; measuring flare frequencies, flare plasma conditions and coronal structures in dozens of active stars; investigate the nature of OB wind shocks; and studying X-ray effects on circumstellar environments.

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