dc.contributor.author | Bhardwaj, A. | en |
dc.contributor.author | Bodewits, D. | en |
dc.contributor.author | Christian, Damian J. | en |
dc.contributor.author | Combi, M.R. | en |
dc.contributor.author | Dennerl, K. | en |
dc.contributor.author | Lepri, S. | en |
dc.contributor.author | Lisse, C.M. | en |
dc.contributor.author | Wolk, Scott J. | en |
dc.contributor.author | Zurbuchen, T.H. | en |
dc.date.accessioned | 2017-12-05T22:06:49Z | |
dc.date.available | 2017-12-05T22:06:49Z | |
dc.date.issued | 2012 | en |
dc.identifier.citation | Astronomische Nachrichten 333(4), 324-334. (2012) | en |
dc.identifier.issn | 0004-6337 | en |
dc.identifier.uri | http://hdl.handle.net/10211.3/198381 | en |
dc.description.abstract | While X-ray astronomy began in 1962 and has made fast progress since then in expanding our knowledge about where in the Universe X-rays are generated by which processes, it took one generation before the importance of a fundamentally different process was recognized. This happened in our immediate neighborhood, when in 1996 comets were discovered as a new class of X-ray sources, directing our attention to charge exchange reactions. Charge exchange is fundamentally different from other processes which lead to the generation of X-rays, because the X-rays are not produced by hot electrons, but by ions picking up electrons from cold gas. Thus it opens up a new window, making it possible to detect cool gas in X-rays (like in comets), while all the other processes require extremely high temperatures or otherwise extreme conditions. After having been overlooked for a long time, the astrophysical importance of charge exchange for the generation of X-rays is now receiving increased general attention. In our solar system, charge exchange induced X-rays have now been established to originate in comets, in all the planets from Venus to Jupiter, and even in the heliosphere itself. In addition to that, evidence for this X-ray emission mechanism has been found at various locations across the Universe. Here we summarize the current knowledge about solar system X-rays resulting from charge exchange processes. | en |
dc.format.extent | 11 pages | en |
dc.language.iso | en | en |
dc.publisher | Astronomische Nachrichten | en |
dc.relation.uri | doi.org/10.1002/asna.201211663 | en |
dc.rights | copyright 2012 Wiley-VCH Verlag GmbH & Co. | en |
dc.subject | solar system X-ray | en |
dc.subject | x-ray | en |
dc.subject | exchange process | en |
dc.title | Solar system X-rays from charge exchange processes | en |
dc.type | Article | en |
dc.identifier.orcid | orcid.org/0000-0003-1746-3020 | en |
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