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

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31#
發(fā)表于 2025-3-26 23:19:31 | 只看該作者
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
32#
發(fā)表于 2025-3-27 04:40:46 | 只看該作者
33#
發(fā)表于 2025-3-27 05:25:41 | 只看該作者
34#
發(fā)表于 2025-3-27 11:20:41 | 只看該作者
Informationsqualit?t von Nachrichtenron R filters within a field of 36 x 36 arcmin, corresponding to about 200 x 200 kpc at the Fornax distance. This is the largest area around this galaxy ever studied with CCD photometry. The cluster system of NGC 1399 is found to extend further than 100 kpc away from the galaxy. The color distributi
35#
發(fā)表于 2025-3-27 15:25:31 | 只看該作者
Informationsquellen der Konsumentenst detailed information on GCSs to date is dominated by the Milky Way and M31 (both spirals) and smaller galaxies within the Local Group. NGC 5128, as the nearest large E galaxy (.), provides an important link to studies of extragalactic GCSs. But its proximity, combined with a moderately low Galact
36#
發(fā)表于 2025-3-27 21:27:14 | 只看該作者
37#
發(fā)表于 2025-3-27 22:53:50 | 只看該作者
38#
發(fā)表于 2025-3-28 05:14:38 | 只看該作者
39#
發(fā)表于 2025-3-28 10:08:10 | 只看該作者
1431-2433 evolution studies. As a whole, the?book gives an up-to-date view of the field at the beginning of the new decade, which will without doubt?again bring significant progress in our understanding of globular cluster systems and galaxy formation and evolution..978-3-642-07339-7978-3-540-45044-3Series ISSN 1431-2433 Series E-ISSN 1611-6143
40#
發(fā)表于 2025-3-28 13:15:55 | 只看該作者
Sichere Kommunikation im Gesundheitswesen,]) were used in this study. 533 sources pass these criteria, and will be referred to as clusters for the remainder of the paper. With this sample we are able to study the cluster formation history, the cluster initial mass function (cIMF), and search for evidence of cluster disruption.
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