The X-ray spectra of the flaring and quiescent states of YZ CMi observed by XMM-Newton
The X-ray spectra of the flaring and quiescent states of YZ CMi observed by XMM-Newton
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XMM-Newton观测到的YZ CMi耀斑态和静止态的X射线谱
DOI：
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发表时间：
2007
期刊：
影响因子：
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通讯作者：
M. Güdel
中科院分区：
文献类型：
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作者：
A. Raassen;U. Mitra;M. Güdel
我们分析的X射线光谱的活动晚型星星YZ CMi（M4.5 V）的静态以及活跃的阶段，我们得到的排放措施（EM）的分布，元素丰度，电子温度和密度，这反过来又被用来估计耀斑环的长度以及日冕磁场强度。
We analyse the X-ray spectrum of the active late-type star YZ CMi (M4.5V); for quiescent as well as active stages, we derive emission measure (EM) distributions, elemental abundances, and electron temperatures and densities, which are in turn used to estimate flare loop lengths as well as coronal magnetic field strengths.