1. INTRODUCTION

2. OBSERVATIONS
2.1. Chandra data
2.2. HST / ACS data

3. X-RAY SPECTRAL PROPERTIES

4. RESULTS
4.1. Candidate accreting binaries
4.2. Other identifications

5. DISCUSSION
5.1. Distance constraints for the CV candidates
5.2. The CV density towards the bulge
5.3. The hard X-ray sources in the central bulge

6. CONCLUSIONS