ARIES-Institutional Digital Repository

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

Show simple item record

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


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search ARIES-IDR


Advanced Search

Browse

My Account

Context