Star Forming Regions and Young Clusters

Details Star Forming Regions and Young Clusters Star Forming Regions and Young Clusters

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..223m&link_type=abstract

Chandra Proposal ID #01200061

Computer Science

Chandra Proposal Id #01200061

Scientific paper

Our observations of star formation regions and young compact clusters will address: i) stellar collapse and commencement of nuclear burning - associated high X-ray activity makes such observations one of the best techniques for selecting young stars in molecular clouds for detailed study; and ii) the question of the existence of the X-ray activity in low mass stars at the onset of full convection - the problem of conflicting evidence arising from studies of field M dwarfs can be addressed by observing young open clusters cores over a range of ages and by examining the behavior of Lx and Lx/L_bol with spectral type and/or rotation.

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