File:JWST Dust NGC7496 II.jpg
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Size of this preview: 735 × 600 pixels. Other resolutions: 294 × 240 pixels | 588 × 480 pixels | 941 × 768 pixels | 1,255 × 1,024 pixels | 1,370 × 1,118 pixels.
Original file (1,370 × 1,118 pixels, file size: 482 KB, MIME type: image/jpeg)
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Summary[edit]
Summary[edit]
| Description |
Adding a new version of NGC7496 to have the same colorization as NGC628 and IC5332. The center of this galaxy has a very bright point source known as an active galactic nucleus (AGN). You can see it's quite different from the other two which do not have an actively accreting black hole. Red (screen layer mode): MIRI F2100W Orange: MIRI F1130W Cyan: MIRI F770W Extra overall brightness in grayscale: MIRI F1000W |
| Date | |
| Source | JWST Dust NGC7496 |
| Author | Judy Schmidt |
Licensing[edit]
This file is licensed under the Creative Commons Attribution 2.0 Generic license.
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This image was originally posted to Flickr by geckzilla at https://flickr.com/photos/54209675@N00/52238754431. It was reviewed on 25 July 2022 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0. |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 17:59, 25 July 2022 | | 1,370 × 1,118 (482 KB) | Fabian RRRR (talk | contribs) | =={{int:filedesc}}== {{Information |Description=Adding a new version of NGC7496 to have the same colorization as NGC628 and IC5332. The center of this galaxy has a very bright point source known as an active galactic nucleus (AGN). You can see it's quite different from the other two which do not have an actively accreting black hole. Red (screen layer mode): MIRI F2100W Orange: MIRI F1130W Cyan: MIRI F770W Extra overall brightness in grayscale: MIRI F1000W |Source=[https://www.flickr.com/p... |
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