1. Charge exchange x-ray emission: Astrophysical observations and potential diagnostics
- Author
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F. Salces Carcoba, D. G. Seely, P. Sauter, P. C. Stancil, M. S. Hokin, A. K. Vassantachart, C. R. Vane, Kelsey M. Morgan, D. J. Nader, M. Fogle, D. McCammon, I. N. Draganic, V.M. Andrianarijaona, Dallas Wulf, S. L. Romano, A. Galindo-Uribarri, C. C. Havener, C. I. Guillen, and X. Defay
- Subjects
Physics ,Astrophysics::High Energy Astrophysical Phenomena ,Comet ,Astronomy ,Astrophysics ,Ion ,Jupiter ,Interstellar medium ,Solar wind ,Physics::Space Physics ,ROSAT ,Astrophysics::Solar and Stellar Astrophysics ,Heliosphere ,Geocorona - Abstract
Interest in astrophysical sources of charge exchange X-rays has been growing steadily since the discovery of X-ray emission from the comet Hyakutake with ROSAT in 1996. Since then, charge exchange has been observed between solar wind ions and neutrals in the geocorona and in the atmospheres of Mars and Jupiter. Charge exchange with interstellar neutrals within the heliosphere between solar wind ions and neutral hydrogen and helium from the interstellar medium is now acknowledged as contributing a considerable (although currently unknown) fraction of the soft X-ray background. We make a brief survey of the heliospheric, Galactic, and extragalactic systems in which charge exchange has been observed or is predicted to take place. Experiments measuring velocity dependent cross-section and line ratios for Lyman-series lines and He-like triplets are needed to check current theoretical models of charge exchange emission and aid interpretation of observations. We point out a number of systems that are of astrophy...
- Published
- 2013