Starburst blown superbubbles: gas metalicity and X-ray emission

Details Starburst blown superbubbles: gas metalicity and X-ray emission Starburst blown superbubbles: gas metalicity and X-ray emission

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3...85s&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 85-90

Computer Science

Scientific paper

The X-ray emission from star forming regions in different types of galaxies is discussed. Special attention is paid to cases with an obvious discrepancy between model predictions and observed X-ray luminosities. A new solution of this problem, based on time dependent calculations of the X-ray emitting gas metalicity, is here given. Our results show that supernovae metal ejection leads to a high overabundance of the hot bubble interior, that allows for up to an order of magnitude higher X-ray luminosities compared with standard predictions.

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