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Large-scale structure of the cosmos / Particle physics / Plasma physics / X-ray astronomy / Dark matter / Active galactic nucleus / International X-ray Observatory / X-ray telescope / Redshift / Physics / Astronomy / Physical cosmology


6 Soft X-ray and ultra-violet metal-line emission from the gas around galaxies The gas around galaxies is diffuse and much fainter than the galaxies themselves. A large fraction of the gas has temperatures between 104.5
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Document Date: 2012-03-13 09:22:05


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City

ASTRO / /

Company

The star / Matsuda / Komatsu / /

IndustryTerm

intergalactic gas / Dilute halo gas / metal-line emission / average gas properties / gas particle / halo gas / hotter gas / gas particles / circumgalactic gas / ultra-violet metal-line emission / brightest metal lines / energy range / metal-line emission traces / gas pressure / gas emissivity scales / halo gas mological simulations / neutral gas / cold gas / diffuse halo gas / energy resolution / dense halo gas / expected metal-line surface brightness / metal lines / diffuse gas / gas cloud / energy / /

MusicGroup

X-ray / /

Organization

International Monetary Fund / /

TVStation

KCWI / /

Technology

radiation / X-ray / microwave / simulation / /

URL

http /

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