File:ESO-Filaments in the Tarantula Nebula-phot-34b-04-fullres.jpg
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Original file (1,628 × 1,422 pixels, file size: 2.49 MB, MIME type: image/jpeg)
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Summary
| Description |
English: Filaments of ionized gas in the proximity of the R136 cluster, which lies beyond the lower left edge of the photo. The different hues are due to different physical conditions that manifest themselves in the spectrum of the light emitted by the gas. Note also the dark lanes running roughly from bottom left to upper right, which are due to filaments of obscuring dust seen in projection against the background of bright nebulosity. The sky field measures 6.5 x 5.7 arcmin. North is up and East is left. |
| Date | |
| Source | http://www.eso.org/gallery/v/ESOPIA/Nebulae/phot-34b-04-fullres.jpg.html |
| Author | ESO |
| Permission (Reusing this file) |
http://www.eso.org/public/outreach/press-rel/copyright.html |
Search for more ESO images at: http://www.eso.org/gallery/v/ESOPIA
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 11:52, 26 June 2009 | | 1,628 × 1,422 (2.49 MB) | Lars Lindberg Christensen | {{Information |Description={{en|1=Filaments of ionized gas in the proximity of the R136 cluster, which lies beyond the lower left edge of the photo. The different hues are due to different physical conditions that manifest themselves in the spectrum of th |
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