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QSR J1819+3845 is a quasar notable for being the most variable known extragalactic radio source. This quasar shows variations of factors of four or more on a timescale of hours.〔Dennett-Thorpe J, de Bruyn AG. (2000). "The Discovery of a Microarcsecond Quasar: J1819+384". The Astrophysical Journal. 2000 Feb 1; 529 (2), L65-L68.〕 The variations have been shown to be due to scattering in the interstellar medium (ISM). This quasar furnished the elegant proof〔Dennett-Thorpe J, de Bruyn AG. (2002). "Interstellar scintillation as the origin of the rapid radio variability of the quasar J1819+3845". Nature. 2002 Jan 3; 415(6867), 57-60.〕 of the role of scattering due to the ISM, or interstellar scintillation, by showing a time delay in arrival between the signal at widely spaced telescopes (in the USA and Netherlands). Interstellar scintillation is the observed effect of interference and refractive phenomena due to the ISM. It can be thought of as the ISM focusing and defocusing the radio waves from the source, producing a pattern of dark and bright patches, rather like light and dark patches at the bottom of a fish pond. As the Earth moves through these patches we observe a temporal variation in the radio intensity (like a fish swimming through light and dark patches). If the standard theory of diffractive scintillation is assumed to apply, ground-based radio traces would seem to require that J1819+3845 contains a component that must be less than about 5 microarcseconds across; this would require its temperature to be in excess of 1015 K. However, the scintillation may perhaps be interpreted as being due to an unusual piece of intervening interstellar medium. Nonetheless, its importance lies in having proved the importance of interstellar scintillation in creating the observed variations in brightness in at least some quasars, which had been the subject of some discussion. == 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「QSR J1819+3845」の詳細全文を読む スポンサード リンク
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