X-rays from charge transfer in astrophysics: Overview

被引：3

作者：

Raymond, J. C. ^{[1
]}

机构：

[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

来源：

ASTRONOMISCHE NACHRICHTEN | 2012年 / 333卷 / 04期

关键词：

atomic processes; X-rays: ISM; X-rays: diffuse background; EMISSION; EXCHANGE;

D O I：

10.1002/asna.201211677

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

X-rays produced by charge transfer provide a major fraction of the soft X-ray background. If they contribute significantly to emission from other astrophysical sources, then model fits that ignore them will yield wrong answers, and an important diagnostic opportunity will be missed. Several recent papers suggest charge transfer contributions to observed X-ray spectra. This informal overview discusses analysis that might confirm the charge transfer interpretation and carry it toward the status of a useful diagnostic. (c) 2012 WILEY-VCH Verlag GmbH&Co. KGaA, Weinheim

引用

页码：290 / 291

页数：2

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