Triggered Star Formation and Diffuse Emssion in Ara OB1

Details Triggered Star Formation and Diffuse Emssion in Ara OB1 Triggered Star Formation and Diffuse Emssion in Ara OB1

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cxo..prop.1394w&link_type=abstract

Chandra Proposal ID #05200622

Computer Science

Chandra Proposal Id #05200622

Scientific paper

We propose deep observations of the unique, nearby (1.3 kpc) and related massive star forming regions NGC 6193 (75 ks) and RCW 108 (100ks) located < 4pc apart. NGC 6193 contains several early O stars which are less than 3 Myr old. The winds from these stars are inducing the star formation in the embedded, < 0.5 Myr, RCW 108 which also contains at least 1 O star. The NGC 6193 O stars offer a unique opportunity to observe the interaction of winds from O stars separated by 13,000 A.U. (10" = 0.06pc). The comparative study of the revealed, older NGC 6193 and the embedded younger RCW 108 cluster, both containing OB stars, will give insight into triggered star formation, diffuse emission in regions of massive star formation, the X-ray evolution of young stars.

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