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The fermi gamma-ray space telescope, exploding stars, neutron stars, and black holes
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Thompson, David J. |
| Copyright Year | 2010 |
| Description | Since August, 2008, the Fermi Gamma-ray Space Telescope has been scanning the sky, producing a full-sky image every three hours. These cosmic gamma-rays come from extreme astrophysical phenomena, many related to exploding stars (supernovae) or what these explosions leave behind: supernova remnants, neutron stars, and black holes. This talk uses sample Fermi results, plus simple demonstrations, to illustrate the exotic properties of these endpoints of stellar evolution. |
| File Size | 26029 |
| Page Count | 1 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20110014330 |
| Archival Resource Key | ark:/13960/t6wx2ch96 |
| Language | English |
| Publisher Date | 2010-04-13 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Gamma Rays Neutron Stars Gamma Ray Telescopes Supernovae Spaceborne Telescopes Explosions Stellar Evolution Black Holes Astronomy Cosmic Rays Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Presentation |