星暴星系M82和NGC3256的电荷交换辐射
Charge-exchange emission in the starburst galaxies M82 and NGC3256
摘要：
电荷交换（CE）发射产生的功能，这是检测与当前的X射线仪器在最明亮的近星系。我们描述了这些方面的恒星形成星系M82和NGC 3256，从朱雀和XMM-牛顿望远镜观测到的X射线光谱。从离子（O，C）和中性（Mg，Si）的发射是公认的。我们还描述了如何在未来的任务微量热计仪器将改善CE观测。
英文摘要：
Charge-exchange (CE) emission produces features which are detectable with the current X-ray instrumentation in the brightest near galaxies. We describe these aspects in the observed X-ray spectra of the star forming galaxies M82 and NGC 3256, from the Suzaku and XMM-Newton telescopes. Emission from both ions (O, C) and neutrals (Mg, Si) is recognised. We also describe how microcalorimeter instrumentation on future missions will improve CE observations.
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