R水瓶座与伽马射线天文学

黄金时代 Pub Date : 2018-06-06 DOI:10.22323/1.315.0062
K. Tanabe, Y. Motizuki
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引用次数: 0

摘要

在南极冰芯中,由于伽马射线的作用,存在许多硝酸盐离子浓度峰值。从日本“富士圆顶”南极站提取的部分冰芯与11世纪相对应,显示出三组尖峰。前两个可能与SN1006和SN1054一致。第三个可能是共生双星金牛座R的爆发(公元1073年和1074年),在古代朝鲜文献中被记录为“客座星”。此外,还存在几个与其他世纪相对应的硝酸盐离子峰。一些没有任何历史记录的峰值可能是由于不可见或缺失的SNe或其他(经典新星或共生恒星)爆发的伽马射线。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
R Aquarii and Gamma Ray Astronomy
In the Antarctic Ice core there exist many nitrate ion concentration spikes due to gamma ray. A part of the ice core extracted from the Japanese Antarctic station named Dome Fuji,corresponding with 11th century, shows three set of spikes.The first two possibly coincide with SN1006 and SN1054.The third one is probably due to the symbiotic binary R Auarii's outbursts (1073 and 1074AD)that were recorded in the ancient Korean documents as a "guest star". Moreover,there exist several nitrate ion spikes corresponding with other centuries. Some of the spikes without any historical records are possibly due to the gamma-ray from invisible or missing SNe or other (classical novae or symbiotic star )outbursts.
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