File:NGC 3190 (noao-n3190mm).tiff
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Size of this JPG preview of this TIF file: 640 × 600 pixels. Other resolutions: 256 × 240 pixels | 960 × 900 pixels.
Original file (960 × 900 pixels, file size: 2.48 MB, MIME type: image/tiff)
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[edit]DescriptionNGC 3190 (noao-n3190mm).tiff |
English: NGC3190, a spiral galaxy of type SA(s)a in the constellation Leo, was imaged during engineering work at the KPNO Mayall 4-meter telescope in January of 2001. The large size of the telescope and the smaller format imager used for test work combine to make the field of view only just the size of the galaxy itself. Multiple exposures on this faint galaxy took a total of 3000s in the blue (B) band, 2000s in green (V) and 1000s in red (R). NGC3190 in fact forms a small group (Hickson 44, Arp 316) with NGC3193 to the east, NGC3187 to the west, and NGC3185, significantly further away to the southwest. Interestingly, NGC3189 refers to the south-west (lower right) part of NGC3190. The strong dust lane down the middle apparently misled the catalog compilers into giving it two separate numbers. NGC3190 also contains an active galactic nucleus. |
Date | 30 June 2020, 21:33:00 (upload date) |
Source | NGC 3190 |
Author | Hillary Mathis/NOIRLab/NSF/AURA |
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[edit]This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public NOIRLab website, along with the texts of press releases, announcements, images of the week and captions; are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. | |
This file is licensed under the Creative Commons Attribution 4.0 International license.
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current | 19:42, 17 September 2023 | 960 × 900 (2.48 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/noao-n3190mm.tif via Commons:Spacemedia |
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Image title | NGC3190, a spiral galaxy of type SA(s)a in the constellation Leo, was imaged during engineering work at the KPNO Mayall 4-meter telescope in January of 2001. The large size of the telescope and the smaller format imager used for test work combine to make the field of view only just the size of the galaxy itself. Multiple exposures on this faint galaxy took a total of 3000s in the blue (B) band, 2000s in green (V) and 1000s in red (R). NGC3190 in fact forms a small group (Hickson 44, Arp 316) with NGC3193 to the east, NGC3187 to the west, and NGC3185, significantly further away to the southwest. Interestingly, NGC3189 refers to the south-west (lower right) part of NGC3190. The strong dust lane down the middle apparently misled the catalog compilers into giving it two separate numbers. NGC3190 also contains an active galactic nucleus. |
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Width | 960 px |
Height | 900 px |
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Compression scheme | Uncompressed |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 2 |
Data arrangement | chunky format |
Software used | @(#)ImageMagick 4.2.9 99/09/01 cristy@mystic.es.dupont.com |