File:M77 H-alpha (15679524440).png
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[edit]DescriptionM77 H-alpha (15679524440).png |
English: Another version of M77 but this time with the H-alpha layer duplicated and set to luminosity mode. This presents the galaxy with an extreme bias towards illuminating the structural details of emissions within the galaxy. More details within the nucleus are also visible. Because the h-alpha data did not cover all parts of the galaxy, I had to crop and rotate the image.
For further information, please see the first version of M77 here. North is NOT up. It is 40.2° counter-clockwise from up. |
Date | Taken on 22 November 2014, 19:33:07 |
Source | M77 H-alpha |
Author | geckzilla |
Flickr sets InfoField | all astronomy; Spirals in Galaxies; Hubble Processing |
Flickr tags InfoField | nebulae; spiral; hst; active; hydrogenalpha; m77; hubble; ngc1068; emission; halpha; seyfert; galaxy; hla |
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@N00/15679524440. It was reviewed on 24 February 2024 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0. |
24 February 2024
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 21:41, 24 February 2024 | 3,532 × 1,929 (11.45 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://live.staticflickr.com/7544/15679524440_842a008d98_o.png via Commons:Spacemedia |
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Date and time of digitizing | 14:33, 22 November 2014 |
File change date and time | 23:31, 23 November 2014 |
Date metadata was last modified | 23:31, 23 November 2014 |
Unique ID of original document | xmp.did:0744deeb-8de6-9440-9c34-801441276bdf |
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