Íomhá: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 picteilín, méid comhaid: 55 KB, cineál MIME: image/gif, looped, 39 frames, 1.6 s)

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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.
Dáta
Foinse Goddard Space Flight Center
Credit: NASA/DOE/Fermi LAT Collaboration
Údar Roger Romani (Stanford University) (Lead), Lucas Guillemot (CENBG), Francis Reddy (SPSYS)

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Public domain Chruthaigh NASA an comhad seo, agus tógadh as suíomh Greasáin NASA nó foilseachán NASA é. Tá gach saothar den saghas sin sa fearann poiblí ach amháin an suaitheantas NASA, mar ní féidir saothair de chuid rialtas cónaidhme Stáit Aontaithe Mheiriceá a chur faoi chóipcheart. Féach ar an leathanach pholasaí cóipchirt NASA nó an leathanach pholasaí íomhanna JPL le tuilleadh eolais.
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faoi láthair09:56, 9 Iúil 2009Mionsamhail do leagan ó 09:56, 9 Iúil 2009226 × 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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