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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Date: 2012-03-13 09:22:05 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 Add to Reading List Source URL: home.strw.leidenuniv.nl Download Document from Source Website File Size: 459,41 KB Share Document on Facebook

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