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根据空间探测器探测1.809 MeV 射线的结果人们断定,银河系内目前存在着2~ 3 M⊙的星际26Al。迄今所建立起的有关天体模型几乎全部无法解决星际26Al的形成问题。有人提出,SNIa是26Al合成的新途径,核反应(16O+14N)可能成为星际26Al的重要天体来源之一。利用AMS技术可以研究16O+14
According to the results of space probe detection of 1.809 MeV rays, it has been concluded that there are 2 ~ 3 M⊙ interstellar 26 Al in the Milky Way. Almost all of the celestial body models so far established can not solve the formation of interstellar 26Al. It was suggested that SNIa is a new pathway for the synthesis of 26Al, and nuclear reaction (16O + 14N) may be one of the important celestial bodies of interstellar 26Al. The use of AMS technology can study 16O +14