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Tidal disruption event : ウィキペディア英語版 | Tidal disruption event A tidal disruption event is an astronomical phenomenon that occurs when a star gets too close to a supermassive black hole's event horizon and is pulled apart by the black hole's tidal forces, experiencing spaghettification.〔(【引用サイトリンク】 title=Tidal Disruption of a Star By a Massive Black Hole )〕 It was first proposed in 1975 that tidal disruption events should be an inevitable consequence of black holes in galaxy nuclei whereas later theorists concluded that the resulting flare of radiation from the accretion of the stellar debris could be a unique signpost for the presence of a dormant black hole in the center of a normal galaxy. == See also ==
* Gamma-ray burst#Tidal disruption events * Super soft X-ray source#Large amplitude outbursts
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「Tidal disruption event」の詳細全文を読む
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