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X-ray emission from clusters and groups of galaxies
Recent major advances in x-ray imaging and spectroscopy of clusters have allowed the determination of their mass and mass profile out to ≈1/2 the virial radius. In rich clusters, most of the baryonic mass is in the gas phase, and the ratio of mass in gas/stars varies by a factor of 2–4. The baryonic...
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
National Academy of Sciences
1998
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| Accesso online: | https://ncbi.nlm.nih.gov/pmc/articles/PMC34193/ https://ncbi.nlm.nih.gov/pubmed/9419327 |
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