chandra_520 August 30th, 2012
Credit: X-ray: NASA/CXC/U.Mich./S.Oey, IR: NASA/JPL, Optical: ESO/WFI/2.2-m
The star cluster NGC 1929 contains massive stars that produce intense radiation, expel matter at high speeds, and race through their evolution to explode as supernovas. The winds and shock waves carve out huge cavities called superbubbles in the surrounding gas. X-rays from Chandra (blue) in this composite image reveal the regions created by these winds and shocks, while infrared data from Spitzer (red) outline where the dust and cooler gas are found. Optical light from an ESO telescope in Chile (yellow) shows where ultraviolet radiation from the young stars is causing the gas to glow.
Provider: Chandra X-ray Observatory
Image Source: http://chandra.harvard.edu/photo/2012/n1929/
Curator: Chandra X-ray Observatory, Cambridge, MA, USA
Image Use Policy: http://chandra.harvard.edu/photo/image_use.html
Telescope | Spectral Band | Wavelength | |
---|---|---|---|
Chandra (ACIS) | X-ray (X-ray) | 826.7 pm | |
Spitzer (IRAC) | Infrared (Near-IR) | 3.6 µm | |
Spitzer (IRAC) | Infrared (Near-IR) | 5.8 µm | |
Spitzer (IRAC) | Infrared (Mid-IR) | 8.0 µm | |
Spitzer (MIPS) | Infrared (Mid-IR) | 24.0 µm | |
ESO (WFI) | Optical (OII) | 372.0 nm | |
ESO (WFI) | Optical (OIII) | 500.0 nm | |
ESO (WFI) | Optical (H-alpha) | 656.0 nm | |
Detailed color mapping information coming soon...
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