Titlebook: Validation Numerics; Theory and Applicati R. Albrecht,G. Alefeld,H. J. Stetter Book 1993 Springer-Verlag/Wien 1993 Fortran.Matrix.algorithm

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Hans-Jürgen Dobneres with new directions to go. New data, new phenomena; but the sentiment was that we were building on a much safer foundation, even if the Universe was unfolding in a much more complex and unexpected way than was previously anticipated. In editing these proceedings a decision was made well in advanc

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A. Frommer,G. Mayers, perhaps because of the recent merging history of the clusters. We also present a recent analysis of population gradients in clusters which suggests that the observed evolution in cluster populations is consistent with a scenario where changing infall rates drive the fraction of star forming galax

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Weimin Han,F. A. Potra in both Li and Be abundances. These stars place strong constraints on the nature and depth of the mixing processes responsible for their light element abundances. The 7th star (HD 160617) shows the remarkable aspect of deficient B, probably deficient Be, and completely normal Li. No stellar destruc

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K.-U Jahnn stars are in that case not metal-rich as previously thought, but they have a metallicity comparable to the LMC, with an age between 0.1–1 Gyr. A significant fraction of the carbon stars still have luminosities fainter than the lower LMC limit of. A similar trend is present among carbon stars found

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