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

被引:10
作者
Pandey, S. B. [1 ]
机构
[1] Aryabhatta Res Inst Observat Sci, Naini Tal 263129, India
关键词
Massive stars; core-collapse; supernovae; gamma-ray bursts; optical; telescopes; HIGH-RESOLUTION SPECTROSCOPY; OPTICAL AFTERGLOW; IBC SUPERNOVA; HOST GALAXY; OBSERVATIONAL CONSTRAINTS; PRESUPERNOVA EVOLUTION; MEASURED METALLICITIES; MASSIVE SINGLE; SHOCK BREAKOUT; LIGHT-CURVE;
D O I
10.1007/s12036-013-9178-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
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.
引用
收藏
页码:157 / 173
页数:17
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