伽瑪射線暴

伽瑪射線暴（英文：Gamma-ray burst，縮寫GRB，又叫伽瑪暴），係來自遙遠星系、能量極高嘅爆炸光芒。伽瑪射線暴係宇宙之中由大爆炸以嚟能量同光度都最高嘅電磁脈衝。^[1]爆發可以持續十毫秒至數個鐘。^[2]^[3]^[4]最初嘅伽瑪射線閃光之後，仲會留低時間更長、波長更長嘅「餘輝」（X光、紫外光、可見光、紅外光、微波、無線電波）。^[5]

參考資料

↑ "Gamma Rays". NASA. 原著喺2012-05-02歸檔.
↑ Atkinson, Nancy (2013-04-16). "New Kind of Gamma Ray Burst is Ultra Long-Lasting". Universe Today (美國英文). 原著喺2023-02-05歸檔. 喺2022-01-03搵到.
↑ Gendre, B.; Stratta, G.; Atteia, J. L.; Basa, S.; Boër, M.; Coward, D. M.; Cutini, S.; d'Elia, V.; Howell, E. J; Klotz, A.; Piro, L. (2013). "The Ultra-Long Gamma-Ray Burst 111209A: The Collapse of a Blue Supergiant?". The Astrophysical Journal. 766 (1): 30. arXiv:1212.2392. Bibcode:2013ApJ...766...30G. doi:10.1088/0004-637X/766/1/30. S2CID 118618287.
↑ Graham, J. F.; Fruchter, A. S. (2013). "The Metal Aversion of LGRBs". The Astrophysical Journal. 774 (2): 119. arXiv:1211.7068. Bibcode:2013ApJ...774..119G. doi:10.1088/0004-637X/774/2/119. S2CID 125987555.
↑ Vedrenne & Atteia 2009

呢篇同天文相關係楔位文。歡迎幫維基百科擴寫佢。

[1] "Gamma Rays". NASA. 原著喺2012-05-02歸檔.

[2] Atkinson, Nancy (2013-04-16). "New Kind of Gamma Ray Burst is Ultra Long-Lasting". Universe Today (美國英文). 原著喺2023-02-05歸檔. 喺2022-01-03搵到.

[3] Gendre, B.; Stratta, G.; Atteia, J. L.; Basa, S.; Boër, M.; Coward, D. M.; Cutini, S.; d'Elia, V.; Howell, E. J; Klotz, A.; Piro, L. (2013). "The Ultra-Long Gamma-Ray Burst 111209A: The Collapse of a Blue Supergiant?". The Astrophysical Journal. 766 (1): 30. arXiv:1212.2392. Bibcode:2013ApJ...766...30G. doi:10.1088/0004-637X/766/1/30. S2CID 118618287.

[4] Graham, J. F.; Fruchter, A. S. (2013). "The Metal Aversion of LGRBs". The Astrophysical Journal. 774 (2): 119. arXiv:1211.7068. Bibcode:2013ApJ...774..119G. doi:10.1088/0004-637X/774/2/119. S2CID 125987555.

[5] Vedrenne & Atteia 2009

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