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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 High-energy astronomy ： ウィキペディア英語版 High-energy astronomy High energy astronomy is the study of astronomical objects that release electromagnetic radiation of highly energetic wavelengths. It includes X-ray astronomy, gamma-ray astronomy, and extreme UV astronomy, as well as studies of neutrinos and cosmic rays. The physical study of these phenomena is referred to as high-energy astrophysics.〔http://highenergyastro.homestead.com/〕 Astronomical objects commonly studied in this field may include black holes, neutron stars, active galactic nuclei, supernovae, supernova remnants, and gamma ray bursts. ==Missions== Some space and ground based telescopes that have studied high energy astronomy include the following:〔http://heasarc.gsfc.nasa.gov/docs/observatories.html〕 *H.E.S.S. *MAGIC *Fermi *AGILE (spacecraft) *INTEGRAL *NuSTAR *XMM-Newton - X-ray Multi-Mirror Mission - Newton *Chandra X-ray Observatory *Suzaku (ASTRO-E) *Swift *AMS-02 *AUGER *TA *IceCube 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「High-energy astronomy」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.