1. Introduction

2. Discovery of a HI Cloud Complex  
2.1. ALFALFA Observations  
2.2. Cloud Morphologies and Kinematics from ALFALFA Data  

3. Aperture Synthesis Follow-up Observations  
3.1. HI Aperture Synthesis Detections  
3.2. HI Morphologies and Kinematics of C1 and C2  
3.3. Non-Detections in the VLA Follow-up Data  

4. CO(3–2) Observations

5. The Environment of the Cloud Complex

6. Discussion  
6.1. Orbital Motion Through the ICM: a Simple Simulation  
6.2. Possible Formation Mechanisms  
6.3. Timing Considerations  
6.4. Evaporation Timescale  

7. Summary