Titlebook: Extragalactic Globular Cluster Systems; Proceedings of the E Markus Kissler-Patig Conference proceedings 2003 Springer-Verlag Berlin Heidel

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https://doi.org/10.1007/978-3-322-84573-3about a decade old. But these star clusters are being studied, individually or as populations, with ever increasing interest. In this review article I will describe some of the reasons for this growing interest and summarize some of the recent findings.

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https://doi.org/10.1007/978-3-322-92382-0This suggests a continuum of cluster properties and a universality in cluster formation mechanisms, which is likely to also include classical “globular” clusters. Comparison with existing data for a sample of galaxies shows that the luminosities of the brightest clusters are consistent with random s

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https://doi.org/10.1007/978-3-322-85741-5heoretical stellar population synthesis models, to obtain age estimates. The accuracy to which this can be done depends on the number of observations through different (broad-band) filters available as well as, crucially, on the actual wavelength range covered. I show, based on the examples of the n

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Innovationen als Unternehmensfunktion,emain-sequence stars down to 1 M.. We do not see any change in the slope of the luminosity function down to the completeness limit anywhere within the observed field. We suggest the flattening seen in the optically derived mass function (MF) around 2 M. claimed by [3] is due to differential reddenin

BROOK

Zur Strukturiertheit von Anwendungsbereichenin the Colour-Magnitude Diagram and the synthetic cluster sequences computed from stellar evolutionary models. In the conventional isochrone fitting procedure, the age is estimated in a subjective way. Here, we calculate the degree of likelihood by applying a modern statistical estimator, the Saha e

青石板

https://doi.org/10.1007/978-3-642-59604-9 cluster system and galaxy formation. Recent . observations have revealed large numbers of low mass X-ray binaries around early type galaxies, a significant fraction of which are associated with globular clusters. I present results from this exciting new field and comment on some of the possibilitie

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