Overview
- Captured by the VLT Survey Telescope at ESO’s Paranal Observatory, the nebula’s silhouette resembles a bat gliding between Circinus and Norma.
- The glowing red emission traces hydrogen ionized by radiation from newly formed stars embedded in the cloud.
- Dense, cooler dust filaments block background starlight, creating the dark, skeletal features seen across the complex.
- RCW 94 outlines the right wing and RCW 95 forms the body, while other portions of the structure lack official designations.
- Spanning an area about four full Moons across, the image was made with the 268‑megapixel OmegaCAM on VST, with publicly accessible survey data from VPHAS+ and VVV.