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Titlebook: Spectral Evolution of Galaxies; Proceedings of the F Cesare Chiosi,Alvio Renzini Conference proceedings 1986 D. Reidel Publishing Company,

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M Giants in the Galactic Nuclear Bulges which are quite rare in the solar neighborhood. It is argued that the large numbers of M giants being found in the Galactic bulge are the best candidates for inclusion in stellar synthesis models for spheroidal systems. These M giants differ systematically in luminosity, color, and CO index from t
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Age and Mass of M Giants in the Galactic Bulgenerally been used in synthesizing population models; a revision in the value of .. accentuates the disparity in luminosity. Luminosities in excess of those of the long-period variables in metal-rich globular clusters are rare. Thus the argument for assigning an age ≤ 2 Gyr to late M bulge giants and
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Age and Mass of M Giants in the Galactic Bulgeerties of the late M giants in the bulge appear to be compatible with an SMR composition and an age in the range 6 to 15 Gyr. The evidence leans toward models in which the star formation rate has been negligible for a considerable part of the total evolution time.
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Conference proceedings 1986tand the evolution of stellar populations. Following an opening session dealing with some outstanding questions of galaxy evolution. Session I addressed the specific problems of galaxy and star formation processes. topics of uncertainty and controversy to which IRAS observations may give novel persp
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0067-0057 I addressed the specific problems of galaxy and star formation processes. topics of uncertainty and controversy to which IRAS observations may give novel persp978-94-010-8543-4978-94-009-4598-2Series ISSN 0067-0057 Series E-ISSN 2214-7985
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J. M. van der Hulst,E. Hummel,W. C. Keel,R. C. Kennicutt Jr.
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Ausharzen von Leder,en, kommt es nicht selten vor, daß harzige, klebrige, flacher oder rundlicher geformte, tropfenförmige Ausscheidungen auf der Narbenseite, manchmal auch Fleischseite oder beiden Seiten des Leders auftreten, daß das Leder „ausharzt“ (Abb. 8).
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Wenn Bildung großgeschrieben wirded intermediate volcanic tuffs and lavas. 61 variability study samples were composed of quartz, feldspar, mica, kaolinite, chlorite with minor pyrite, arsenopyrite, jarosite and accessories. Multivariate statistics of mineral composition and multi-element assays distinguished following ore types: (1
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