File:The radial velocities of the Balmer lines in WD 0931+444 (geminiann14006c).tiff
From Wikimedia Commons, the free media repository
Jump to navigation
Jump to search
The_radial_velocities_of_the_Balmer_lines_in_WD_0931+444_(geminiann14006c).tiff (500 × 478 pixels, file size: 100 KB, MIME type: image/tiff)
File information
Structured data
Captions
Summary
[edit]DescriptionThe radial velocities of the Balmer lines in WD 0931+444 (geminiann14006c).tiff |
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 |
Other versions |
|
Licensing
[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.
|
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 17:15, 23 October 2023 | 500 × 478 (100 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/geminiann14006c.tif via Commons:Spacemedia |
You cannot overwrite this file.
File usage on Commons
The following page uses this file:
Metadata
This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Image title | 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. |
---|---|
Width | 500 px |
Height | 478 px |
Bits per component |
|
Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 174 |
Horizontal resolution | 150 dpi |
Vertical resolution | 150 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop 21.2 (Windows) |
File change date and time | 18:53, 25 July 2020 |
Exif version | 2.31 |
Color space | Uncalibrated |