eso_eso2209a June 15th, 2022
Credit: ESO, ALMA (ESO/NAOJ/NRAO)/Wong et al., ESO/M.-R. Cioni/VISTA Magellanic Cloud survey. Acknowledgment: Cambridge Astronomical Survey Unit
This composite image shows the star-forming region 30 Doradus, also known as the Tarantula Nebula. The background image, taken in the infrared, is itself a composite: it was captured by the HAWK-I instrument on ESO’s Very Large Telescope (VLT) and the Visible and Infrared Survey Telescope for Astronomy (VISTA), shows bright stars and light, pinkish clouds of hot gas. The bright red-yellow streaks that have been superimposed on the image come from radio observations taken by the Atacama Large Millimeter/submillimeter Array (ALMA), revealing regions of cold, dense gas which have the potential to collapse and form stars. The unique web-like structure of the gas clouds led astronomers to the nebula’s spidery nickname.
Provider: European Southern Observatory
Image Source: https://www.eso.org/public/images/eso2209a/
Curator: European Southern Observatory, Garching bei München, None, Germany
Image Use Policy: Creative Commons Attribution 4.0 International License
Telescope | Spectral Band | Wavelength | |
---|---|---|---|
ALMA (Band 6) | Millimeter (12CO) | 1.3 mm | |
VLT (HAWK-I) | Infrared (Y) | 1.0 µm | |
VLT (HAWK-I) | Infrared (Ks) | 2.1 µm | |
Visible and Infrared Survey Telescope for Astronomy (VIRCAM) | Infrared (Y) | 1.0 µm | |
Visible and Infrared Survey Telescope for Astronomy (VIRCAM) | Infrared (J) | 1.3 µm | |
Visible and Infrared Survey Telescope for Astronomy (VIRCAM) | Infrared (Ks) | 2.2 µm | |
VLT (HAWK-I) | Infrared (Ks) | 2.1 µm | |
VLT (HAWK-I) | Infrared (Y) | 1.0 µm | |
ALMA (Band 6) | Millimeter (13CO) | 1.4 mm | |
Detailed color mapping information coming soon...
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