Abstract
AbstractCharge‐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 (© 2012 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
