XMM-Newton Proposal 02042203

Details XMM-Newton Proposal 02042203 XMM-Newton Proposal 02042203

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..225k&link_type=abstract

XMM-Newton Proposal ID #02042203

Computer Science

Cg303138, Sa101Cg6, Cg4Sa101, Xmm-Newton Proposal 02042203

Scientific paper

We propose one 30 ksec and two 15 ksec EPIC imaging of triggered star forming regions (SFRs), CG30/31/38 and CG4/6/SA101. These SFRs represent a different star forming environment compared to well known SFRs, such as Orion or Taurus. The molecular clouds are evaporating due to the radiation from high mass stars that are not as close as O stars in Orion, but at moderate distances (tens to 100 pc). Although we have sampled a group of PMS stars from our HRI imaging, optical, IR photometry, and spectroscopy, we are most likely seeing only the tip of a larger PMS population yet to be discovered. These proposed EPIC imaging will sample more complete census of PMS stars providing valuable data set to study different environments of triggered star formation.

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