File:NGC5216, NGC5218 - Noao-arp-104.jpg
![File:NGC5216, NGC5218 - Noao-arp-104.jpg](https://upload.wikimedia.org/wikipedia/commons/thumb/9/9f/NGC5216%2C_NGC5218_-_Noao-arp-104.jpg/800px-NGC5216%2C_NGC5218_-_Noao-arp-104.jpg?20211113115225)
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Summary
[edit]DescriptionNGC5216, NGC5218 - Noao-arp-104.jpg |
English: Arp 104 Keenan’s System (NGC 5216 & NGC 5218)
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Date | June 30, 2020, 9:33 p.m. | ||||
Source | https://noirlab.edu/public/images/noao-arp-104/ | ||||
Author |
Credit: T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOIRLab/NSF/AURA) |
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Permission (Reusing this file) |
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File history
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 11:52, 13 November 2021 | ![]() | 2,936 × 1,952 (1.85 MB) | Fabian RRRR (talk | contribs) | == {{int:filedesc}} == {{Information |description={{en|1='''Arp 104 Keenan’s System (NGC 5216 & NGC 5218) This image was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory. Arp 104, also known as Keenan’s System, consists of the two spiral galaxies NGC 5216 (bottom) and NGC 5218 (top). The two are connected by a thin stream of gas, in which new stars are forming. The stream was created when the two galaxies passed by each... |
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Headline | None |
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Credit/Provider | T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOIRLab/NSF/AURA) |
Source | NSF's NOIRLab |
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Usage terms |
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Date and time of data generation | 21:33, 30 June 2020 |
Software used | Adobe Photoshop CS6 (Macintosh) |
File change date and time | 10:01, 14 May 2015 |
Date and time of digitizing | 04:45, 25 May 2013 |
Date metadata was last modified | 02:01, 14 May 2015 |
Unique ID of original document | xmp.did:C4F53273044568118C149D54520DA144 |
Keywords |
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Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |
IIM version | 4 |