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Core-Collapse Supernovae and Gamma-Ray Bursts in TMT Era

机译:TMT时代的核塌陷超新星和伽马射线爆发

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摘要

Study of energetic cosmic explosions as a part of time domain astronomy is one of the key areas that could be pursued with upcoming Giant segmented optical-IR telescopes with a very large photon collecting area applying cutting edge technology. Existing 8-10 m class telescopes have been helpful to improve our knowledge about core-collapse supernovae, gamma-ray bursts and nature of their progenitors and explosion mechanisms. However, many aspects about these energetic cosmic explosions are still not well-understood and require much bigger telescopes and back-end instruments with high precision to address the evolution of massive stars and high-redshift Universe in more detail. In this presentation, possible thrust research areas towards core-collapse supernovae and gamma-ray bursts with the Thirty-Meter Telescope and back-end instruments are presented.
机译:作为时域天文学的一部分,高能宇宙爆炸的研究是即将出现的,采用尖端技术的,具有非常大的光子收集面积的巨型分段光学红外望远镜可以追求的关键领域之一。现有的8-10 m级望远镜有助于提高我们对核塌陷超新星,伽马射线爆发及其祖先性质和爆炸机制的了解。但是,关于这些高能宇宙爆炸的许多方面仍未得到很好的理解,需要更大型的望远镜和高精度的后端仪器才能更详细地处理大质量恒星和高红移宇宙的演化。在本演示中,介绍了使用三十米望远镜和后端仪器对核塌陷超新星和伽马射线爆发的可能推力研究领域。

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