Overview
- Herbig-Haro 49/50, located 630 light-years away in the Chamaeleon I Cloud complex, is a protostellar outflow driven by the young star Cederblad 110 IRS4.
- Webb's imaging identified glowing hydrogen and carbon monoxide molecules, energized dust grains, and arc-shaped features tracing the jet's impact on its surroundings.
- The previously unclear 'fuzzy object' at the tip of the outflow was revealed to be a distant face-on barred-spiral galaxy with regions of active star formation.
- The Chamaeleon I Cloud complex, where HH 49/50 resides, offers insights into environments similar to where the Sun likely formed.
- The Webb Telescope, a collaboration between NASA, ESA, and CSA, showcases advancements in infrared imaging and international scientific cooperation.