Computer Science
Scientific paper
Mar 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop....3s&link_type=abstract
XMM-Newton Proposal ID #02000302
Computer Science
Chaii - Field 1, Chaii - Field 2, Xmm-Newton Proposal 02000302
Scientific paper
We propose for XMM-Newton observations of two highly extincted fields in the ChaII star forming region. Our aim is to complete the census of cloud members using X-ray emission as a means to discover young stars. A clear assessment of the full stellar population is essential to establish the evolutionary state of a star forming cloud. ChaII seems to represent a comparatively young phase where many stars retain their disks. But a large number of low-mass members may still be hidden in the dark parts of the cloud. In contrast to earlier X-ray instrumentation XMM-Newton provides enough sensitivity and an extended spectral range allowing to penetrate the highly absorbed parts of ChaII, and study the stellar population across regions of high and varying extinction.
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