THE DISTRIBUTION OF BARYON MATTER IN THE NEARBY X-RAY GALAXY CLUSTERS
We present the results on the distribution of baryon matter in the galaxy clusters (z < 0.2), based on the Chandra X-ray Observatory data. The observed surface brightness profiles were approximated by β- model, which provides a good fit for all clusters. We found a correlation between cluster...
| Auteurs principaux: | , |
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| Format: | Article |
| Langue: | English |
| Publié: |
Odessa I. I. Mechnykov National University
2012-11-01
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| Collection: | Odessa Astronomical Publications |
| Accès en ligne: | http://oap.onu.edu.ua/article/view/83328 |