tóng-àn:Cycle of pulsed gamma rays from the Vela pulsar.gif
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Cycle_of_pulsed_gamma_rays_from_the_Vela_pulsar.gif （226 × 169 siōng-sò͘ , tóng-àn chiàm-liōng: 55 KB, MIME luī-hêng: image/gif, 循環, 39 畫格, 1.6秒）
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Khài-iàu
| Soat-bêng |
English: This image shows pulsed gamma rays from the Vela pulsar as constructed from photons detected by Fermi's Large Area Telescope. The Vela pulsar, which spins 11 times a second, is the brightest persistent source of gamma rays in the sky. The bluer colour in the latter part of the pulse indicates the presence of gamma rays with energies exceeding a billion electron volts (1 GeV). For comparison, visible light has energies between two and three electron volts. Red indicates gamma rays with energies less than 300 million electron volts (MeV); green, gamma rays between 300 MeV and 1 GeV; and blue shows gamma rays greater than 1 GeV. The image frame is 30 degrees across. The background, which shows diffuse gamma-ray emission from the Milky Way, is about 15 times brighter here than it actually is. |
| Ji̍t-kî | |
| Chhut-chhù |
Goddard Space Flight Center Credit: NASA/DOE/Fermi LAT Collaboration |
| Chok-chiá | Roger Romani (Stanford University) (Lead), Lucas Guillemot (CENBG), Francis Reddy (SPSYS) |
Siū-khoân
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本作品由NASA創作，屬於公有領域。根據NASA的版權政策：“NASA的創作除非另有聲明否則不受版權保護。”（參見：Template:PD-USGov/zh，NASA版權政策或JPL圖像使用政策） |  |
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| Ji̍t-kî/Sî-kan | 細張圖 | 寸尺 | Iōng-chiá | Chù-kái | |
|---|---|---|---|---|---|
| hiān-chāi | 2009-nî 7-goe̍h 9-ji̍t (pài-sì) 09:56 | | 226 × 169（55 KB） | Originalwana | {{Information |Description={{en|1=This imgae shows pulsed gamma rays from the Vela pulsar as constructed from photons detected by Fermi's Large Area Telescope. The Vela pulsar, which spins 11 times a second, is the brightest persistent source of gamma ray |
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