Titlebook: Globular Clusters - Guides to Galaxies; Proceedings of the J Tom Richtler,Søren Larsen Conference proceedings 2009 Springer-Verlag Berlin H

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https://doi.org/10.1007/978-3-0348-0018-1a of their integrated light. To do this, we are using a “training set” of spatially resolved clusters. We scan these clusters to obtain integrated light spectra, and also take spectra of individual stars in these clusters to obtain “fiducial” abundances by the usual analysis methods. We briefly desc

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Sectionally Complemented Latticeservations of GC turnoff stars that these abundance anomalies were already present in the gas from which the observed stars formed. This provides undisputed support to the so-called self-enrichment scenario according to which a large fraction of GC low-mass stars have formed from material processed t

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Mathematics and Its Applicationsandardized protocols, they can be useful for research through appropriate tools developed either by the host facility or by the science end users. These data holdings also have enormous potential for educational purposes from pre-college through non-majors courses and expert course curricula in univ

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Sydney Bulman-Fleming,Kenneth McDowell are naturally reproduced by the presence of super-He-rich populations. However, there are no isochrones and self-consistent HB tracks available in the literature that are based on the up-to-date input physics and wide ranges of He and metal abundances. Here we present new sets of .. isochrones and

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https://doi.org/10.1007/978-3-211-33614-4 and reliable observational datasets (broadband BVI photometry) available for the cluster, both for variable and nonvariable stars, to infer the most likely masses of individual horizontal branch stars by comparison against theoretical evolutionary tracks, suitably transformed to the observational p

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https://doi.org/10.1007/978-3-663-20491-6ter Survey (ACSVCS) – to observe 100 early-type members of the Virgo Cluster using the .. The properties of the nuclei from this survey are compared with those of the globular clusters. A similar comparison between the nuclei and the supermassive black holes found in many massive galaxies points to

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