SS-433/W50 at TeV Energies
| dc.creator | Rowell, G. P. | |
| dc.creator | Collaboration, HEGRA | |
| dc.date | 2001-04-17 | |
| dc.date.accessioned | 2026-07-07T01:58:15Z | |
| dc.date.available | 2026-07-07T01:58:15Z | |
| dc.description | The HEGRA CT-System was used to search for TeV gamma-rays from the microquasar and supernova remnant combination SS-433/W50 over the 1998 and 1999 observing seasons, resulting in about 20 hours of useful data. An analysis of various extended sources of location guided by X-Ray observations reveals no evidence for TeV emission at photon energies above 1 TeV, with resulting 99% upper limits in the range 8 to 10 of the Crab flux. For one of these locations, the eastern jet termination, a model predicting a presently detectable TeV gamma-ray flux via the inverse Compton upscattering of microwave background photons is now somewhat constrained. The results and model contraints are briefly discussed. | |
| dc.description | 8 pages, 2 figures, to appear in proceedings of 'Similarities and Universality in Relativistic Flows' Mykonos, Greece, Oct 2000 (http://pluto.mpi-hd.mpg.de/theory/surf/) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0104288 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0104288 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2696 | |
| dc.subject | Astrophysics | |
| dc.title | SS-433/W50 at TeV Energies | |
| dc.type | text |