1 INTRODUCTION
2 DATA
2.1 Ultraviolet
2.2 Optical
2.3 Infrared
3 DATA REDUCTION
4 MODELING
5 DETECTION OF STAR-FORMING REGIONS
6 RESULTS
7 DISCUSSION
7.1 Implications for Dust Composition
7.2 Comparison to Gordon et al. (2003)
7.3 Recent Star Formation History
8 SUMMARY