| dc.contributor.author | Pandey, S. B. | |
| dc.date.accessioned | 2015-06-10T10:04:15Z | |
| dc.date.available | 2015-06-10T10:04:15Z | |
| dc.date.issued | 2013 | |
| dc.identifier.uri | http://hdl.handle.net/123456789/1109 | |
| dc.description.abstract | 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 super- novae, gamma-ray bursts and nature of their progenitors and explosion mechanisms. However, many aspects about these energetic cosmic explo- sions 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 presen- tation, possible thrust research areas towards core-collapse supernovae and gamma-ray bursts with the Thirty-Meter Telescope and back-end instruments are presented. | en_US |
| dc.language.iso | en_US | en_US |
| dc.publisher | Indian Academy of Sciences | en_US |
| dc.relation.ispartofseries | jaa34-157 | |
| dc.subject | Massive stars—core-collapse—supernovae—gamma-ray bursts—optical—telescopes. | en_US |
| dc.title | Core-Collapse Supernovae and Gamma-Ray Bursts in TMT Era | en_US |
| dc.type | Article | en_US |