File:NGC 346 2008.jpg

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Captions

Captions

Star-forming region NGC 346

Summary

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Description
English: This new portrait of the bright star-forming region NGC 346, in which different wavelengths of light swirl together like watercolours, reveals new information about how stars form. NGC 346 is located 210,000 light-years away in the Small Magellanic Cloud, a neighbouring dwarf galaxy of the Milky Way. The image is based on data from ESA XMM-Newton (X-rays; blue), ESO's New Technology Telescope (visible light; green), and NASA's Spitzer (infrared; red). The infrared light shows cold dust, while the visible light denotes glowing gas, and the X-rays represent very hot gas. Ordinary stars appear as blue spots with white centres, while young stars enshrouded in dust appear as red spots with white centres.
Date
Source https://www.eso.org/public/images/eso0834a/
Author ESO/ESA/ JPL-Caltech/NASA/ D. Gouliermis (MPIA) et al.

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current22:32, 7 February 2021Thumbnail for version as of 22:32, 7 February 2021700 × 661 (100 KB)777burger (talk | contribs)Uploaded a work by ESO/ESA/ JPL-Caltech/NASA/ D. Gouliermis (MPIA) et al. from https://www.eso.org/public/images/eso0834a/ with UploadWizard

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