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LS I +61 303 is a binary system harboring a compact object and a massive star (possibly a microquasar) that emits ''HE'' and ''VHE'' (High Energy and Very High Energy) gamma rays. It is only one of three known star systems that produce such energetic rays. The other two systems are PSR B1259-63 and LS 5039. ==References== * * (Variable Very High Energy Gamma-ray Emission from the Microquasar LS I +61 303 ) * (SCIENCE Journal ) - Submitted on March 31, 2006 - Accepted on May 8, 2006 * * (Variable Very High Energy Gamma-Ray Emission from the Microquasar LS I +61 303 ) ABSTRACT * (PDF ) Published online May 18, 2006; 10.1126/science.1128177 (Science Express Reports) * (Variable Very-High-Energy Gamma-Ray Emission from the Microquasar LS I +61 303 ) SUPPORT 抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「LS I +61 303」の詳細全文を読む スポンサード リンク
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