| gamma-ray burst | has duration 0.1 - 4 s |  |
| has distribution isotropic with an increase towards the galactic center |  |
| has frequency of occurrence 5 per year |  |
| has energy spectrum 0.1-1.2 MeV |  |
| is a part of celestial sphere |  |
| has discovery date July 2, 1967 |  |
| has definition Short, intense, low-energy bursts, first recorded by the Vela satellite system on 1967 July 2. Their isotropic distribution suggests an extragalactic origin, but a galactic disk origin cannot be ruled out: there is a large increase in γ-ray flux in the direction of the galactic center. |  |
| is a kind of gamma ray source |  |
| gamma ray source | has wavelength gamma ray |  |
| celestial body | has spectra |  |
| physical object | has location or center of gravity |  |
| has angular momentum |  |
| has mass |  |
| has velocity |  |
| has momentum |  |
| has temperature |  |
| has volume |  |
| has extent |  |
| has material |  |