On the role of radioactive decays in powering gamma rays and X-rays from novae

On the role of radioactive decays in powering gamma rays and X-rays from novae
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放射性衰变在为新星伽马射线和 X 射线提供动力方面的作用

DOI:
10.1086/171573
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发表时间:
1992
期刊:
The Astrophysical Journal
影响因子:
--
通讯作者:
J. Truran
J. Truran
中科院分区:
--
文献类型:
--
作者:
M. Livio;A. Mastichiadis;H. Oegelman;J. Truran

文献摘要

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现有的新星爆发x射线辐射模型遇到了一些困难。计算了由放射性衰变产生的伽马射线的康普顿衰变可能产生的x射线通量。它特别证明了22 Na的放射性衰变可能在硬x射线的产生中起着有趣的作用,特别是在富含氧、氖和镁的新星中
Existing models for X-ray emission from novae in outburst encounter several difficulties. The X-ray flux that may be expected to result from Compton degradation of gamma rays produced by radioactive decays is calculated. It is demonstrated specifically that radioactive decays of 22 Na may play an interesting role in the production of hard X-rays, particularly in novae enriched in oxygen, neon, and magnesium