File:The radial velocities of the Balmer lines in WD 0931+444 (geminiann14006c).jpg
The_radial_velocities_of_the_Balmer_lines_in_WD_0931+444_(geminiann14006c).jpg (500 × 478 pixels, file size: 65 KB, MIME type: image/jpeg)
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editDescriptionThe radial velocities of the Balmer lines in WD 0931+444 (geminiann14006c).jpg |
English: The radial velocities of the Balmer lines in WD 0931+444. The bottom panel shows all of these data points phased with the best-fit period. The dotted line represents the best-fit model for a circular orbit with a period of 19.8 minutes. |
Date | 16 June 2014, 14:06:00 (upload date) |
Source | The radial velocities of the Balmer lines in WD 0931+444 |
Author | International Gemini Observatory/NOIRLab/NSF/AURA |
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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. | |
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current | 17:15, 23 October 2023 | 500 × 478 (65 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/geminiann14006c.jpg via Commons:Spacemedia |
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Credit/Provider | International Gemini Observatory/NOIRLab/NSF/AURA |
Source | NSF's NOIRLab |
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Date and time of data generation | 14:06, 16 June 2014 |
Software used | Adobe Photoshop CS3 Macintosh |
File change date and time | 18:53, 25 July 2020 |
Unique ID of original document | uuid:4BBE3E3C63F4E311B97DB5EF75FB2F79 |
Date and time of digitizing | 22:01, 12 June 2014 |
Date metadata was last modified | 13:53, 25 July 2020 |
Copyright status | Copyright status not set |
Keywords | WD 0931+444 |
Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |
IIM version | 4 |