翻訳と辞書 Words near each other ・ PSR B1257+12 ・ PSR B1257+12 A ・ PSR B1257+12 B ・ 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 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 J0357+3205 ： ウィキペディア英語版 PSR J0357+3205 PSR J0357+3205 is a pulsar is located about 1,600 light years from Earth.〔(【引用サイトリンク】publisher=NASA )〕 PSR J0357+3205 was originally discovered by the Fermi Gamma-ray Space Telescope in 2009.〔 ==X-ray Bright Tail== A very long, X-ray bright tail (over 4 light years across) may be stretching away from PSR J0357+3205.〔 The tail is puzzling because it shares characteristics with other tails extending from pulsars, but differs in certain properties. If the tail is at the same distance as the pulsar then it stretches for 4.2 light years in length.〔 This would make it one of the longest X-ray tails ever associated with a so-called "rotation- powered" pulsar, a class of pulsar that get its power from the energy lost as the rotation of the pulsar slows down. (Other types of pulsars include those driven by strong magnetic fields and still others that are powered by material falling onto the neutron star.) 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 J0357+3205」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.