1. Introduction

2. The data
2.1. Herschel/SPIRE observations, data reduction and flux extraction
2.2. Dust mass estimate
2.3. Ultraviolet, optical and HI data

3. The dust-to-stellar mass ratio

4. The dust-to-HI mass ratio

5. Discussion
5.1. The origin of the dust scaling relations
5.2. Dust stripping

6. Summary