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- W4245018448 abstract "X-ray emissions from clusters are most likely originated from a thin hot plasma in a collisional ionization equilibrium. The optical depth of continuum component is order of 10 –3 , whereas that of emission lines is around unity. Present emission models used for spectral fitting can not estimate this effect, so that the determination of elemental abundances seems to include large uncertainty. The high resolution spectroscopy with ASCA gives a clue to investigate the physical state of hot intracluster gas and a impact to reconsider the basic atomic processes. This is important issue to deeply understand the structure, formation and evolution of clusters, and the origin of intracluster gas." @default.
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- W4245018448 modified "2023-09-26" @default.
- W4245018448 title "ASCA observations of clusters of galaxies" @default.
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- W4245018448 doi "https://doi.org/10.1017/s0074180900081122" @default.
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