| タイトル | Gamma rays of 0.3-30 MeV from PSR0833 - 45 |
| 著者（英） | Long, J.; White, R. S.; Oneill, T.; Dayton, B.; Zych, A.; Tumer, O. T. |
| 著者所属（英） | California Univ.|California State Univ. |
| 発行日 | 1984-07-19 |
| 言語 | eng |
| 内容記述 | Pulsed gamma rays from the Vela pulsar PSR0833 - 45 are reported for the first time over the medium energy range 0.3-30 MeV. They were observed with a double scatter gamma-ray telescope flown on a balloon over Australia on Nov. 10, 1981, 31 days after a large glitch in the pulsar period. The first and second pulses were detected from single scatters in the top scintillators at energies over 0.3 MeV with statistical significances of 1.6 sigma each, and by double scatters from all detector cell pairs at energies of 1-30 MeV with significance of 4.8 sigma and 3.8 sigma. The phase separation of the two pulses is 0.43 + or - 0.02 at the same absolute phases previously found by SAS2 and COS B for energies over 35 MeV. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 84A43786 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/396862 |
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