伽玛射线暴宿主星系的宇宙演化

S. Savaglio
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摘要

由于其极端的亮度,伽马射线暴(GRBs)可以在星系的敌对区域,附近和非常高的红移中被探测到,使它们成为重要的宇宙探测器。对长时间伽马射线暴(其前身是一颗大质量恒星)所在星系的研究证明了它们与恒星形成的联系。尽管如此,与星系总数的联系仍然存在争议,主要是因为统计数字很小:迄今为止探测到的grb约为1100个,测量到的红移约为280个,详细研究的宿主约为70个。这些典型的低红移(z > 4)很少被探索,但达到的深度限制指向非常小的和恒星形成的物体,类似于低z人口。这种“回到未来”的行为是长伽马射线暴与宇宙年轻区域恒星形成联系的自然结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
THE COSMIC EVOLUTION OF GAMMA-RAY BURST HOST GALAXIES
Due to their extreme luminosities, gamma-ray bursts (GRBs) can be detected in hostile regions of galaxies, nearby and at very high redshift, making them important cosmological probes. The investigation of galaxies hosting long-duration GRBs (whose progenitor is a massive star) demonstrated their connection to star formation. Still, the link to the total galaxy population is controversial, mainly because of the small-number statistics: ~1, 100 are the GRBs detected so far, ~280 those with measured redshift, and ~70 the hosts studied in detail. These are typically low-redshift (z  > 4) is poorly explored, but the deep limits reached point towards very small and star-forming objects, similar to the low-z population. This “back to the future” behavior is a natural consequence of the connection of long GRBs to star formation in young regions of the universe.
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