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 |