翻訳と辞書 Words near each other ・ PSR B1257+12 C ・ PSR B1259-63/LS 2883 ・ PSR B1509-58 ・ PSR B1620-26 ・ PSR B1620-26 b ・ PSR B1828-11 ・ PSR B1829−10 ・ PSR B1913+16 ・ PSR B1919+21 ・ PSR B1937+21 ・ PSR J0108-1431 ・ PSR J0348+0432 ・ PSR J0357+3205 ・ PSR J0437-4715 ・ PSR J0537-6910 ・ PSR J0540-6919 ・ PSR J0737-3039 ・ PSR J0738-4042 ・ PSR J0855-4644 ・ PSR J1311–3430 ・ PSR J1614–2230 ・ PSR J1719-1438 ・ PSR J1719-1438 b ・ PSR J1748-2446ad ・ PSR J1903+0327 ・ PSR J1951+1123 ・ PSR J2007+2722 ・ PSR J2124-3358 ・ PSR J2144-3933 ・ PSRC1 Dictionary Lists mini英和辞書 mini和英辞書 Webster 1913 Latin-English FOLDOC Wikipedia English ウィキペディア

翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク PSR J0540-6919 ： ウィキペディア英語版 PSR J0540-6919 PSR J0540-6919〔 (PSR B0540-69)〔 is a pulsar in the Tarantula Nebula of the Large Magellanic Cloud. It is the first extragalactic gamma-ray pulsar discovered.〔 〕 ==History== This Crab-like pulsar was first discovered in X-rays in 1984 and subsequently detected at radio wavelengths. Astronomers initially attributed the glow to collisions of subatomic particles accelerated in the shock waves produced by supernova explosions, and it took more than six years of observations by Fermi's Large Area Telescope to detect gamma-ray pulsations from J0540-6919.〔 In 2015, it was determined that J0540-6919 is responsible for about half of the gamma-ray flux from the Tarantula Nebula in the Large Magellanic Cloud. It was identified as a bright source of gamma radiation early in the Fermi mission. 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「PSR J0540-6919」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.