High Energy Emission from the Young Massive Cluster RCW 38

Details High Energy Emission from the Young Massive Cluster RCW 38 High Energy Emission from the Young Massive Cluster RCW 38

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cxo..prop..760w&link_type=abstract

Chandra Proposal ID #03200546

Computer Science

Chandra Proposal Id #03200546

Scientific paper

Taking advantage of Chandra's unique capabilities, we propose to study the youngest, most embedded, massive cluster studied to date in X-rays - RCW 38. The immediate goals of this project are the identification of the embedded PMS stellar population, the investigation of the X-ray properties of the individual class 0-III sources (~10 class 0 & I protostars) and the derivation of a XLF for an extremely young (~0.5 Myr) massive cluster. We will derive the gas-to-dust ratio and its variations towards hundreds of lines of sight across the cluster. Complementary NIR data already taken with the VLT, which probe approximately the same cloud depths, allow an unique multi-wavelength description of a massive star formation episode and its consequences to the surrounding interstellar medium.

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