2-Channel RCW 49
NASA/JPL-Caltech/E. Churchwell (University of Wisconsin) · Download full size image
This image of prolific star-forming region RCW 49 exposes breathtaking detail of this dark and dusty region, which is home to more than 2,200 stars. Shown here in two channels, 3.6 microns mapped as cyan and 4.5 microns mapped as red, dusty organic molecules called polycyclic aromatic hydrocarbons (PAHs) glow in the warmth of the starlight. At 4.5 microns, hot hydrogen gas glows very brightly, much like a neon light glowing in visible light, and can be prominently seen in the image.
Posted on: 25 Dec, 2008
- Hubble Space Telescope
- Chandra X-ray Observatory
- Compton Gamma-Ray Observatory
- ROSAT X-ray Observatory
- SOHO Solar Observatory
- WMAP
- 2MASS Sky Survey
- ASTER Earth Imaging Instrument
- MISR Earth Imaging Instrument
- NRAO Gallery
- NAOJ Subaru Telescope
- Galaxy Evolution Explorer (GALEX)
- European Southern Observatory (ESO)
- Wide-Field Imager (WFI)
- SOFI Infrared Multi-mode Instrument
- Canada-France-Hawaii Telescope (CFHT)
- New Technology Telescope (NTT)
- Atacama Pathfinder Experiment (APEX)
- SOHO Daily Images - 1996
- Spitzer Space Telescope (SIRTF)
- Infrared Legacy Gallery
Latest Thoughts
Computer Games for Seniors
Smokeless Tobacco Criticized
Starting School Later Prevents Car Crashes
Why Weather Changes Make People Sick
FDA Issues Diet Pill Warning



























































































































































































































































































































































