1 INTRODUCTION
1.1 NGC 3607 and NGC 3608 in the Leo II group

2 DATA
2.1 Observations and reduction techniques
2.2 Photometry

3 GLOBULAR CLUSTER SELECTION

4 DEFINING THE GC SYSTEMS OF EACH GALAXY
4.1 Surface brightness method
4.2 Major axis method
4.3 Analysis of kinematic data

5 ANALYSIS OF PHOTOMETRIC DATA
5.1 GC system of NGC 3607
5.2 GC system of NGC 3608

6 DISCUSSION
6.1 GC system distribution and galaxy effective radius
6.2 GC system ellipticity and galaxy ellipticity
6.3 GC metallicity gradients and galaxy stellar mass
6.4 Ratio of blue to red GCs with environment density and galaxy mass
6.5 Formation of GC systems

7 CONCLUSIONS