1 INTRODUCTION

2 THE SAMI GALAXY SURVEY  
2.1 Data quality and S/N cuts  
2.2 Spectral classification  

3 DEFINING 1- AND MULTI-COMPONENT GALAXIES  
3.1 General properties of 1- and multi-component galaxies  

4 MATCHED SAMPLE ANALYSIS  
4.1 Matched sample analysis results  

5 CORRELATION ANALYSIS

6 IS THE PRESENCE OF MULTIPLE EMISSION LINE COMPONENTS DRIVEN BY STAR FORMATION ON LOCAL OR GLOBAL SCALES?  
6.1 How important is clumpiness?  

7 DISCUSSION  
7.1 Physical interpretation  
7.2 Observational biases