File:Galactic Center in Thermal IR (gemini-20080825-galactic-center-abu-0001).tiff
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Galactic_Center_in_Thermal_IR_(gemini-20080825-galactic-center-abu-0001).tiff (512 × 512 pixels, file size: 862 KB, MIME type: image/tiff)
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DescriptionGalactic Center in Thermal IR (gemini-20080825-galactic-center-abu-0001).tiff |
English: The center of our Milky Way Galaxy showing emission from hot gas that will either form stars or feed the supermassive black hole at the center of our galaxy. Technical Details: The image quality for this Brackett-alpha (hydrogen) line image is FWHM=0.35 arcsec. This image was obtained with the "Abu" thermal-infrared camera built by the National Optical Astronomy Observatory. |
Date | 1 September 2004 (upload date) |
Source | Galactic Center in Thermal IR |
Author | International Gemini Observatory/NOIRLab/Abu Team |
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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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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 18:14, 17 December 2023 | 512 × 512 (862 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/gemini-20080825-galactic-center-abu-0001.tif via Commons:Spacemedia |
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Image title | The center of our Milky Way Galaxy showing emission from hot gas that will either form stars or feed the supermassive black hole at the center of our galaxy. Technical Details: The image quality for this Brackett-alpha (hydrogen) line image is FWHM=0.35 arcsec. This image was obtained with the "Abu" thermal-infrared camera built by the National Optical Astronomy Observatory. |
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Author | Gemini Observatory |
Width | 512 px |
Height | 512 px |
Bits per component |
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Compression scheme | Uncompressed |
Pixel composition | RGB |
Image data location | 26,980 |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 512 |
Bytes per compressed strip | 786,432 |
Horizontal resolution | 244 dpi |
Vertical resolution | 244 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop Lightroom |
File change date and time | 14:40, 28 August 2008 |
Exif version | 2.21 |