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Charge-exchange emission in the starburst galaxies M82 and NGC3256

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.

preprint2012arXivOpen access
Piero Ranalli
astro-ph.HE
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Piero Ranalli

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