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30 Doradus, Diffuse Gamma Ray Source, LAT Image
Description:
Fermi's Large Area Telescope (LAT) shows that an intense star-forming region in the Large Magellanic Cloud named 30 Doradus is also a source of diffuse gamma rays. Brighter colors indicate larger numbers of detected gamma rays. The Tarantula Nebula (also known as 30 Doradus) is an H II region in the Large Magellanic Cloud (LMC). It was originally thought to be a star, but in 1751 Nicolas Louis de Lacaille recognized its nebular nature. 30 Doradus has at its centre the star cluster NGC 2070 which includes the compact concentration of stars known as R136 that produces most of the energy that makes the nebula visible.
Credit:
NASA/DOE/Fermi LAT Collaboration/Science Source
Unique identifier:
SS2738407
Legacy Identifier:
JE4692
Type:
Image
Size:
3750px × 3750px (~40 MB)
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