Fitxategi:Sn2006gy light curve.jpg
Nabigaziora joan
Bilaketara joan
Aurreikuspen honen neurria: 800 × 540 pixel. Bestelako bereizmenak: 320 × 216 pixel | 640 × 432 pixel | 1.024 × 691 pixel | 1.280 × 864 pixel | 3.000 × 2.025 pixel.
Jatorrizko fitxategia (3.000 × 2.025 pixel, fitxategiaren tamaina: 421 KB, MIME mota: image/jpeg)
| Deskribapena |
English: Original caption: "This graph shows the intrinsic brightness of SN 2006gy and how it changes over time. The graphic also demonstrates how much brighter SN 2006gy is when compared to typical examples of the two main supernova classes. Type Ia supernovas involve the thermonuclear explosion of a white dwarf and type II supernovas are the collapse of a massive star. The famous supernova SN 1987A is also shown. Not only does SN 2006gy get much brighter than other supernovas but it stays very bright for much longer." Français : « Ce graphique montre la brillance intrinsèque de SN 2006gy et comment celle-ci change dans le temps (...) » |
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| Data | Data ezezaguna | ||
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| Egilea | NASA/CXC/UC Berkeley/N.Smith et al. | ||
| Lizentzia (Fitxategi hau berrerabiltzen) |
Images credited first to NASA/CXC are in the public domain.
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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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Fitxategiaren historia
Data/orduan klik egin fitxategiak orduan zuen itxura ikusteko.
| Data/Ordua | Iruditxoa | Neurriak | Erabiltzailea | Iruzkina | |
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| oraingoa | 00:20, 10 maiatza 2007 | | 3.000 × 2.025 (421 KB) | wikimediacommons>Tom | {{Information |Description=Original caption: "This graph shows the intrinsic brightness of SN 2006gy and how it changes over time. The graphic also demonstrates how much brighter SN 2006gy is when compared to typical examples of the two main supernova |
Fitxategiaren erabilera
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