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翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク Kilonova ： ウィキペディア英語版 Kilonova A kilonova (also called a ‘macronova’ or an ‘r-process supernova’) occurs when two neutron stars or a neutron star and a black hole merge. Strong electromagnetic radiation is emitted due to the decay of heavy r-process ions that are produced and ejected fairly isotropically during the merger process—similar to a faint, short-lived supernova. A kilonova is thought to be the result of merging of two compact objects, namely a black hole and neutron star, in a binary system. The inspiral and merging of these compact objects are thought to be a strong source of gravitational waves (GWs). It is also thought to be the progenitor of short gamma-ray bursts〔〔 and the predominant source of stable r-process elements in the Universe.〔 == See also == 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「Kilonova」の詳細全文を読む スポンサード リンク 翻訳と辞書 : 翻訳のためのインターネットリソース Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.