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Gamma Ray Study on High Energy Phenomena of Celestial objects

天体高能现象的伽马射线研究

基本信息

批准号：
08044057
负责人：
KIFUNE Tadashi
金额：
$ 4.16万
依托单位：
The Univ.of Tokyo
依托单位国家：
日本
项目类别：
Grant-in-Aid for international Scientific Research
财政年份：
1996
资助国家：
日本
起止时间：
1996 至 1997
项目状态：
已结题

来源：
https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-08044057/
关键词：
Gamma Ray Astronomy Pulsar Supernova Remnant Active Galactic Nuclei Origin of Cosmic Rays Sources of High Energy Gamma Rays Air Cerenkov Lights Gamma Ray Telescope

项目摘要

Our preceding study before the year 1995 has enabled us (i) to commence operation of our 3.8m telescope of imaging Cerenkov lights for gamma ray detection, in 1992 the next year of the launching of Compton gamma ray satellite, (ii) to prove the powerful efficiency of high resolution camera by using the camera of the highest angular resolution until 1996, (iii) to show the ability of observations at large zenith angles for detecting very high energy gamma rays in 10-100 TeV region from the data observing the Crab from the southern hemisphere. Based on these technical development, we have discovered 1 TeV gamma rays from PSR B 1706-44.The results obtained in 1997 are : (1) Very high energy gamma rays (-1TeV) are emitted from a region displaced from the Vela pulsar position by about 0.1ﾟ, which is consistent with the position where the pulsar was born. By comparing the observed gamma ray intensity with X-ray's, the magnetic field in the emission region is estimated as weak as 4muG.(2) The energy spectrum of gamma rays from the Crab nebula is found to continue at least up to 50 TeV,which are the gamma rays of the highest energy that have ever been detected.(3) Very high energy gamma rays has been detected from a supernova remnant SN1006. The result demonstrates that the gamma rays are produced by about 100 TeV electrons, providing a direct evidence that these electrons are shock-acceletated in the north-east rim of the supernova remnant. (4) A hint of 1 TeV gamma rays has been obtained from a gamma ray pulsar PSR B 1509-58. The data in the last year (of a higher threshold energy) shows no indication of signal, suggesting a steep energy spectrum. (6) Other objects, such as a gamma ray burst, the Galactic center Sgr A^<**>, several active galactic nuclei, unidentified EGRET sources and close X-ray binaries, are observed in the 1997 fiscal year. The data are now under analysis.

我们在1995年之前的研究使我们能够(i)在康普顿伽马射线卫星发射的第二年1992年开始使用我们的3.8米切伦科夫成像望远镜进行伽马射线探测，（ii）在1996年之前使用最高角度分辨率的相机来证明高分辨率相机的强大效率。（iii）展示大天顶角观测从南半球观测蟹状星云的资料中探测10-100 TeV区域高能伽马射线的能力。基于这些技术发展，我们从PSR B 1706-44中发现了1 TeV的伽马射线。1997年获得的结果是：(1)从船帆座脉冲星位置偏移约0.1‰的区域发射出高能伽马射线（-1TeV），这与脉冲星的诞生位置一致。将观测到的伽马射线强度与x射线强度进行比较，估计发射区的磁场弱至4muG。(2)蟹状星云的伽马射线能谱至少持续到50 TeV，这是迄今为止探测到的能量最高的伽马射线。从超新星遗迹SN1006中探测到高能伽马射线。结果表明，伽马射线是由大约100 TeV的电子产生的，这为这些电子在超新星遗迹的东北边缘受到冲击加速提供了直接证据。(4)从伽玛射线脉冲星PSR B 1509-58中获得了1 TeV伽马射线的提示。去年的数据（更高的阈值能量）没有显示出信号，表明能量谱陡峭。(6)其他天体，如伽马射线暴、银河系中心Sgr a ^<**>、几个活动星系核、不明EGRET源和近x射线双星，在1997财政年度被观测到。这些数据目前正在分析中。