Microquasars as High-energy Gamma-ray Sources
Microquasars as High-energy Gamma-ray Sources
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作为高能伽马射线源的微类星体
DOI：
10.1088/1009-9271/5/s1/121
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发表时间：
2004
期刊：
影响因子：
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通讯作者：
J. Paredes
中科院分区：
文献类型：
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作者：
J. Paredes
银河微类星体无疑是高能天体物理学领域的最新成员之一，在过去十年中吸引了越来越多的兴趣。然而，微类星体光谱的高能部分是最不为人所知的，这主要是由于过去缺乏灵敏的仪器。微类星体现在是所有在x射线和伽马射线领域工作的天文台的主要目标。它们也可能与康普顿-格罗卫星上的EGRET实验探测到的一些不明高能伽马射线源相对应。本文综述了迄今为止获得的主要观测结果，并总结了目前高能γ射线产生的设想。
Galactic microquasars are certainly one of the most recent additions to the field of high energy astrophysics and have attracted increasing interest over the last decade. However, the high energy part of the spectrum of microquasars is the most poorly known, mainly due the lack of sensitive instrumentation in the past. Microquasars are now primary targets for all of the observatories working in the X-ray and gamma-ray domains. They also appear as the possible counterparts for some of the unidentified sources of high-energy gamma-rays detected by the experiment EGRET on board the satellite COMPTON-GRO. This paper provides a general review of the main observational results obtained up to now as well as a summary of the scenarios for production of high-energy γ-rays at the present moment.
低/硬态银河黑洞双星的朱雀宽带观测
DOI：
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发表时间：
2008
期刊：
影响因子：
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作者：
K. Aamodt;et al.;Uchimura Yasuhiro;Hisayuki Torii for the ALICE Collaboration;Motohashi Hozumi;Saltoh Noriko;Hisayuki Torii for the ALICE-P HOS Collaboration;Baba Daichi;鳥井 久行;鳥井 久行;鳥井 久行;Jun Hatakeyama;Jun Hatakeyama;Hiromi Hirata;Ryoichiri Kageyama;Jun Hatakeyama;Joung Hee Beak;Jun Hatakeyama;畠山 淳;Jun Hatakeyama;Jun Hatakeyama;Jun Hatakeyama;Jun Hatakeyama;Ryoichiro Kageyama;Hiromitsu Takahashi;A. A. Abdo;高橋 弘充;高橋 弘充;高橋弘充;高橋弘充;Hiromitsu Takahashi;Hiromitsu Takahashi;高橋弘充;Hiromitsu Takahashi
通讯作者：
Hiromitsu Takahashi