{ "id": "1601.05958", "version": "v1", "published": "2016-01-22T11:07:38.000Z", "updated": "2016-01-22T11:07:38.000Z", "title": "Plasma code for astrophysical charge exchange emission at X-ray wavelengths", "authors": [ "Liyi Gu", "Jelle Kaastra", "A. J. J. Raassen" ], "comment": "Accepted for publication in Astronomy & Astrophysics", "categories": [ "astro-ph.HE", "astro-ph.EP", "astro-ph.GA", "astro-ph.IM", "physics.atom-ph" ], "abstract": "Charge exchange X-ray emission provides unique insights into the interactions between cold and hot astrophysical plasmas. Besides its own profound science, this emission is also technically crucial to all observations in the X-ray band, since charge exchange with the solar wind often contributes a significant foreground component that contaminates the signal of interest. By approximating the cross sections resolved to $n$ and $l$ atomic subshells, and carrying out complete radiative cascade calculation, we create a new spectral code to evaluate the charge exchange emission in the X-ray band. Comparing to collisional thermal emission, charge exchange radiation exhibits enhanced lines from large-$n$ shells to the ground, as well as large forbidden-to-resonance ratios of triplet transitions. Our new model successfully reproduces an observed high-quality spectrum of comet C/2000 WM1 (LINEAR), which emits purely by charge exchange between solar wind ions and cometary neutrals. It demonstrates that a proper charge exchange model will allow us to probe remotely the ion properties, including charge state, dynamics, and composition, at the interface between the cold and hot plasmas.", "revisions": [ { "version": "v1", "updated": "2016-01-22T11:07:38.000Z" } ], "analyses": { "keywords": [ "astrophysical charge exchange emission", "plasma code", "x-ray wavelengths", "charge exchange x-ray emission", "proper charge exchange model" ], "publication": { "doi": "10.1051/0004-6361/201527615" }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1416618 } } }