The LMC as a QSO Absorption Line System

Details The LMC as a QSO Absorption Line System The LMC as a QSO Absorption Line System

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11692h&link_type=abstract

HST Proposal ID #11692. Cycle 17

Computer Science

Scientific paper

We propose to obtain high resolution, high signal-to-noise observations of QSOs behind the Large Magellanic Clouds. These QSOs are situated beyond the star forming disk of the galaxy, giving us the opportunity to study the distribution of metals and energy in regions lacking significant star formation. In particular, we will derive the metallicities and study the ionization characteristics of LMC gas at impact parameters 3-17 kpc. We will compare our results with high-z QSO absorption line systems.;

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