翻訳と辞書 Words near each other ・ PSR B0943+10 ・ PSR B0950+08 ・ 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 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 J0108-1431 ： ウィキペディア英語版 PSR J0108-1431 PSR J0108-1431 is a solitary pulsar located at a distance of about 130 parsecs (424 light years) in the constellation Cetus. This pulsar was discovered in 1994 during the Parkes Southern Pulsar Survey. It is considered a very old pulsar with an estimated age of 166 million years and a rotation period of 0.8 seconds.〔 The rotational energy being generated by the spin-down of this pulsar is and the surface magnetic field is . As of 2008, it is the second faintest known pulsar. An X-ray emission with an energy flux of was detected in the 0.3–8 keV band using the Chandra X-ray Observatory. This X-ray energy is generated from the conversion of 0.4% of the pulsar's spin-down power. As of 2009, PSR J0108-1431 is the least powerful of the ordinary pulsars that have been detected in the X-ray range. The "Very Large Telescope" at the European Southern Observatory in Northern Chile observed a possible optical counterpart of this neutron star. The object has an apparent magnitude that is (X ≤ 27.8).〔 No companions have been discovered in orbit around this object.〔 ==References== 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 J0108-1431」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.