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

Needlework

https://doi.org/10.1007/978-3-663-08569-0 and determine the ages of globular cluster (sub-)populations. First results indicate that the different galaxies host from little to significant intermediate-age populations, and that the latter have .-element over iron ratios closer to solar than the old population that show an .-element enhancement similar to the diffuse stellar light.

Initiative

Star Clusters in Mergers,about 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.

流逝

The H Band Luminosity Function of the Centre of the 30 Dor Cluster,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 reddening within the cluster, and thus may be spurious.

夾死提手勢

A New Cluster Sub-Population in Lenticular Galaxies,tra, we have shown conclusively that these objects are star clusters associated with their respective galaxies and that they have no known analogs in the MW or elsewhere in the Local Group. These “faint fuzzies” define a new parameter space that must be accommodated in cluster formation models.

Entropion

Generator

話

Austausch universit?rer Kernsystemecluster formation. Empirically it appears that globular cluster formation occurs preferentially in regions in which star formation occurs at a high rate and efficiency. Further, the interstellar medium in such regions is likely to be at a higher pressure than less active star-forming environments. A

landmark

https://doi.org/10.1007/978-3-322-91097-4ependence of the evolution of the mass function of globular cluster systems (GCMF) and of the number of surviving clusters on the properties of the host galaxies. Our simulations include the effects of two-body relaxation, dynamical friction, stellar evolution and the effects of the presence of the

Occlusion

,Kommunikationssysteme zur Datenübertragung,d in a very simple way from the age and mass histograms of large homogeneous samples of clusters with reliable age and/or mass determinations. We demonstrate the method and derive the values of .. and . from cluster samples in selected fields of four galaxies: M51, M33, SMC and the solar neighbourho

祖?zhèn)?/a>

Sichere Kommunikation im Gesundheitswesen,made in five broad band filters; f336w (U), f439w (B), f555w (V), f675w (R), f814w (I), and transformed to the closest corresponding Cousins-Johnson filter magnitude using the equations defined by Holtzmann [5]. Only sources that were found in every filter were analysed. By comparing the spectral en