... the most likely population membership ( halo, thick, or thin disk) for each star in the GC sample using the method outlined in the Appendix and then plotting them in the Galactic tangential velocity VYmetallicity [ Fe/ H ] plane as in Figure 16 ...
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Ссылки http://www.mso.anu.edu.au/~charley/papers/GretherLineweaver2007.pdf -- 693.4 Кб -- 04.11.2007 Похожие документы
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