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Дата изменения: Fri Feb 2 12:03:53 2007
Дата индексирования: Mon Oct 1 21:28:14 2012
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Поисковые слова: arp 220
Population of Galactic globular clusters, figures



FIGURE. 10.—Dependence of cluster metallicity on (a) Galactocentric distance and (b) distance from the Galactic plane. The filled and open circles correspond to the young and old halos, respectively, and the straight lines are the corresponding rms regressions. The small square shows the old-halo cluster excluded from computations based on a 3σ criterion.
discussion in the text | privious figure | next figure