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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| Publicado no: | Proc Natl Acad Sci U S A |
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| Autor principal: | |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
National Academy of Sciences
1998
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC34193/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/9419327/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.95.1.72 |
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