The Nature of the Luminous Starburst Knots in NGC1068 and Their Surrounding Interstellar Medium

Computer Science

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Hst Proposal Id #3852

Scientific paper

We propose to use the FOS to observe bright and luminous starburst knots within the inner 3 Kpc region of NGC 1068. The FOS G130H and G190H spectra of the knots will be modeled with our population synthesis code, which incorporates a new library of high dispersion IUE stellar spectra. The resulting models produce real spectra at a resolution of 0.25A. The use of this powerful new tool, in conjuntion with ~ 3A resolution data from the FOS and complementary ground-based data, will place strong constraints on the stellar ages and the star formation history in the knots.

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