File:GamRayEclipseG22.jpg
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| Description |
English: An orbiting star begins to eclipse its partner, a rapidly rotating, superdense stellar remnant called a pulsar, in this illustration. The pulsar emits multiwavelength beams of light that rotate in and out of view and produces outflows that heat the star’s facing side, blowing away material and eroding its partner. |
| Date | January 26, 2023 |
| Source | https://svs.gsfc.nasa.gov/14281 |
| Author | NASA/Sonoma State University, Aurore Simonnet |
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This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) |  |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 13:16, 10 July 2023 | | 1,800 × 1,200 (1.07 MB) | Юрий Д.К. (talk | contribs) | Uploaded a work by NASA/Sonoma State University, Aurore Simonnet from https://svs.gsfc.nasa.gov/14281 with UploadWizard |
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