The Solar Wind Charge-eXchange Contribution to the Local Soft X-ray BackgroundModel to Data Comparison in the 0.1–1.0 keV Band

被引：0
作者：
Dimitra Koutroumpa
Rosine Lallement
Vasili Kharchenko
Alex Dalgarno
机构：
[1] UMR 7620,
[2] IPSL/Service d’Aéronomie,undefined
[3] CNRS,undefined
[4] Université Pierre et Marie Curie,undefined
[5] Université Versailles-Saint-Quentin,undefined
[6] UMR 7620,undefined
[7] IPSL/Service d’Aéronomie,undefined
[8] Harvard-Smithsonian Center for Astrophysics,undefined
来源：
Space Science Reviews | 2009年 / 143卷
关键词：
SWCX; Heliosphere; SXRB; ISM; Local bubble;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
The major sources of the Soft X-ray Background (SXRB), besides distinct structures as supernovae and superbubbles (e.g. Loop I), are: (i) an absorbed extragalactic emission following a power law, (ii) an absorbed thermal component (∼2×106 K) from the galactic disk and halo, (iii) an unabsorbed thermal component, supposedly at 106 K, attributed to the Local Bubble and (iv) the very recently identified unabsorbed Solar Wind Charge-eXchange (SWCX) emission from the heliosphere and the geocorona.
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页码：217 / 230
页数：13
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