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arXiv 1009.2113astro-ph.GAastro-ph.HE
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用XMM-牛顿法寻找磁星静止时的回旋散射

Search for cyclotron absorptions from magnetars in the quiescence with XMM-Newton

Mykola Malygin, Dmytro Iakubovskyi

摘要:

在这项工作中,我们执行的XMM-牛顿卫星观测到的候选磁星光谱的吸收特性的详细分析。没有发现明显的线状特征,这一否定的结果表明可能存在消除吸收特征的机制。

英文摘要:

In this work, we perform the detailed analysis of absorption features in spectra of magnetar candidates observed by XMM-Newton satellite. No significant line-like feature has been found. This negative result may indicate the possible presence of smoothing out the absorption features mechanisms.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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