Hard X-Ray Search from Class 0 Protostars

Details Hard X-Ray Search from Class 0 Protostars Hard X-Ray Search from Class 0 Protostars

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..136k&link_type=abstract

Chandra Proposal ID #01200704

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Chandra Proposal Id #01200704

Scientific paper

We propose to observe the Orion Molecular Clouds, OMC 2 and OMC 3, with the ACIS-I instrument. With ASCA, these regions are found to exhibit hard X-ray emissions, possiblly from embedded Class 0 and Class I protostars. Our goal is to investigate; (1) when a star begins to emit X-rays, (2) what is the difference in X-rays (spectrum and time variability) between Class 0 and Class I, and the other phases of star formation (ClassII, III), and (3) what is the X-ray emission mechanism in the protostar phase.

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