Talk Title: High Spectral Resolution Evolutionary Synthesis Models
Abstract: New developments (Line Blanketing+NLTE) in the model atmospheres and high spectral resolution Kurucz models are used to built an UV-Optical stellar library that is implemented in an evolutionary synthesis code. The models cover from far-UV to 7000 A, with a spectral sampling of 0.3 A, and metallicities from 2 to 1/10 solar.
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