翻訳と辞書 Words near each other ・ SH2 domain ・ Sh2-1 ・ Sh2-101 ・ Sh2-106 ・ Sh2-2 ・ Sh2-264 ・ Sh2-54 ・ SH2B1 ・ SH2B2 ・ SH2B3 ・ SH2D1A ・ SH2D1B ・ SH2D2A ・ SH2D3A ・ SH2D3C ・ SGR 1627-41 ・ SGR 1806-20 ・ SGR 1900+14 ・ SGR J1550-5418 ・ SGR J1745-2900 ・ SGR Repeal and Medicare Provider Payment Modernization Act of 2014 ・ Sgraffito ・ Sgrech ・ Sgript Cymru ・ Sgro ・ Sgroppino ・ SgrS RNA ・ SGS ・ SGS (New Zealand) Ltd v Quirke Export Ltd ・ SGS Essen 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 SGR 1627-41 ： ウィキペディア英語版 SGR 1627-41 SGR 1627-41, is a soft gamma repeater (SGR), located in the constellation of Ara. It was discovered June 15, 1998 using the Burst and transient Source Experiment (BATSE) and was the first soft gamma repeater to be discovered since 1979. During a period of 6 weeks, the star bursted approximately 100 times, and then went quiet. The measured bursts lasted an average of 100 milliseconds, but ranged from 25 ms to 1.8 seconds. AGR 1627-41 is a persistent X-ray source. It is located at a distance of 11 kpc in the radio complex CTB 33, a star forming region that includes the supernova remnant G337.0-0.1. This object is believed to be a neutron star that undergoes random outbursts of hard and soft X-rays. This may be caused by the loss of angular momentum of a highly magnetized neutron star, or magnetar. Alternatively, it may be a quark star, although this is considered less likely. After the 1998 outburst and the 40-day afterglow, SGR 1627-41 has remained dormant and is steadily cooling down from the peak during the event. ==References== * ( XMM-Newton observation of the Soft Gamma Ray Repeater SGR 1627-41 in a low luminosity state ) 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「SGR 1627-41」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.