File:NGC 4111 (48313336137).png

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Original file(1,422 × 1,536 pixels, file size: 2.38 MB, MIME type: image/png)

Captions

Captions

Five years ago I processed this galaxy, but it was from an older WFPC2 dataset.

Summary

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Description
English: Five years ago I processed this galaxy, but it was from an older WFPC2 dataset. I was checking up on the latest releases to the archive and recognized this fancy little lenticular enigma and decided to revisit it in its latest iteration, this time from WFC3/UVIS & IR. It does take a bit of harsh processing to help bring out the dust detail, but I feel that the destructive nature of such processing is outweighed by the benefit of clarity. Anyway, I really enjoy the way the ring of dust encircles the nucleus of the galaxy perpendicularly to the disk. Everyone has their history.

Data from the following proposal were used to create this image: Addressing a Bias in the Galaxies with Black Hole Mass Measurements

Luminosity: Average of WFC3/UVIS F814W & WFC3/UVIS F475W Red: WFC3/IR F160W Green: WFC3/UVIS F814W Blue: WFC3/UVIS F475W

North is 5.28° counter-clockwise from up.
Date Taken on 18 July 2019, 03:55:17
Source NGC 4111
Author geckzilla
Flickr sets
InfoField
all astronomy; Hubble Processing
Flickr tags
InfoField
polar; disk; perpendicular; ring; lenticular; galaxy; dust; smooth

Licensing

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w:en:Creative Commons
attribution
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@N00/48313336137. It was reviewed on 2 March 2024 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

2 March 2024

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Date/TimeThumbnailDimensionsUserComment
current12:18, 2 March 2024Thumbnail for version as of 12:18, 2 March 20241,422 × 1,536 (2.38 MB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://live.staticflickr.com/65535/48313336137_06569c2461_o.png via Commons:Spacemedia

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