1. INTRODUCTION  
2. SAMPLE AND STELLAR PROPERTIES  
2.1. IR Data  
2.2. Spectral Types  
2.3. Stellar Properties  
3. FAR ULTRAVIOLET EMISSIONS  
3.1. HST Data  
3.2. FUV Line Fitting  
3.3. FUV Continuum Emission  
3.4. Line-Line Correlations  
4. ROTATION-ACTIVITY RELATION  
4.3. Trends with Formation Temperature  
4.4. Alternatives to Rossby Number?  
5. TEMPORAL EVOLUTION  
5.1. UV Emissions Across Time  
5.2. Accumulated UV Evolutionary Histories  
6. CONCLUSIONS