Gamma-ray emission from 134Ce and levels in 134La
โ Scribed by R.C. Greenwood; R.J. Gehrke; R.G. Helmer; C.W. Reich; J.D. Baker
- Publisher
- Elsevier Science
- Year
- 1976
- Tongue
- English
- Weight
- 841 KB
- Volume
- 270
- Category
- Article
- ISSN
- 0375-9474
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
Cosmic rays up to at least 10 15 eV (PeV) are believed to be emitted by Galactic sources, such as supernova remnants. However, no conclusive evidence of their acceleration has been found yet. A trace of ongoing cosmic-ray acceleration is the gamma-ray emission produced by these highly energetic part
The new galactic gamma-source (neutron star) 2129+47XR is detected at energy > 0.8 TeV with flux (0.19 ยฑ 0.09) ร 10 -12 cm -2 s -1 and indices of the integral spectra are kฮณ = -1.12 ยฑ 0.06, kON = -1.28 ยฑ 0.07 and k Of f = -1.73 ยฑ 0.07. The results of ten-year observation of galactic source Cygnus X-