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- W2102709128 abstract "Photometric properties (effective surface brightness, effective radius, radial profile index, axis ratio, color, color gradient) of 328 galaxies in the Coma cluster fainter than ; most of these are found to be old and to have intermediate metal abundance, suggesting that they are nucleated dwarf ellipticals. On the other hand, we find a significant gradient in color, in the sense that galaxy colours become bluer with increasing distance from the cluster center. We conclude that this color gradient represents a metallicity gradient.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html" @default.
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- W2102709128 date "2004-03-01" @default.
- W2102709128 modified "2023-10-16" @default.
- W2102709128 title "Photometric properties of dwarf galaxies in the Coma cluster: radial dependence" @default.
- W2102709128 doi "https://doi.org/10.1017/s1743921304000900" @default.
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