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| has gloss | eng: SN 2005gj was a supernova located approximately 864 million light years (265 million parsecs) away from Earth. It was discovered on September 29, 2005, by the Sloan Digital Sky Survey and the Nearby Supernova Factory. 2005gj was noted because it had qualities of both type Ia and type IIn supernovae, and because hydrogen emission lines were found in its spectrum (see hydrogen spectral series). However, 2005jgs CSM interaction was much stronger and more clearly observed than 2002ics. The mass-loss history 2005gj's hydrogen lines suggest has been cited as evidence that Luminous Blue Variable (LBV) hypergiants can be progenitors of thermonuclear supernovae. |
| lexicalization | eng: SN 2005 gj |
| lexicalization | eng: SN 2005gj |
| lexicalization | eng: SN2005 gj |
| lexicalization | eng: SN2005gj |
| instance of | (noun) a star that explodes and becomes extremely luminous in the process supernova |
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