Historical records of re-explosions of supernovae

Wang Jian-min
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引用次数: 2

Abstract

Of the supernovae recorded in history, there are at least two for which re-explosions have been documented. One is the supernova which appeared on 1006 May 1 (Northern Song Dynasty, Reign Jingde, Year 3) in the asterism Qiguan, south of the lunar mansion Di, which, after 10 years, in 1016 May (Reign Dazhongxiangfu, Year 9) was recorded to have “re-appeared”. The other is the object which appeared by the side of the asterism Tianjiang of the (sixth) lunar mansion Wei (the object known in the West as Kepler's supernova), and which after 60 years in 1664 was again recorded as undergoing an explosion. Therefore, for some type of supernovae, there should exist a mechanism of re-explosions.

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超新星再爆炸的历史记录
在历史上有记录的超新星中,至少有两颗有再爆炸的记录。一颗超新星于公元1006年5月1日(北宋景德三年)出现在月宫帝以南的祁官星群,10年后的1016年5月(大仲祥福九年)被记载为“再次出现”。另一个是出现在月球第六宫魏天江星群旁边的天体(西方称为开普勒超新星的天体),60年后的1664年,它再次被记录为经历了一次爆炸。因此,对于某些类型的超新星,应该存在一种再爆炸的机制。
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Subject index Errata Author index Supernova remnants of known age and X-radiation The effect of an ellipsoidal distribution of star velocities on galactic density waves
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