Search for X-Rays from Collapsing Magnetized Pre-Stellar Condensations

Details Search for X-Rays from Collapsing Magnetized Pre-Stellar Condensations Search for X-Rays from Collapsing Magnetized Pre-Stellar Condensations

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..547g&link_type=abstract

Chandra Proposal ID #02200277

Computer Science

Chandra Proposal Id #02200277

Scientific paper

X-rays from young protostars are likely, as is the VLA emission, a reliable tracer of the start of an accretion process onto a central object. We seek to assess whether or not X-ray emission is simultaneous with the very first steps of star formation, or even precedes them. The main goal of this proposal is to search for X-ray emission from collapsing pre-stellar condensations, and to investigate the chronology between X-ray, VLA emission, and outflow phenomena during protostar formation. We request 2 x 100 ksec to study the double NGC 2068/2071 complex in the Orion B giant molecular cloud at d~400 pc, containing several young protostars, and many newly discovered pre-stellar condensations.

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