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

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Informationsqualit?t von Nachrichten. The cluster system contains . clusters and the specific frequency is found to be . in the V band. NGC 1399 shows a pronounced color gradient, which can be interpreted by field populations that are genuinely related to the red and the blue cluster populations.

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The ,-Function Applied to the Age of Globular Clusters,idence level of 99%, we find that the best estimate of the age is 14.0 Gyr within the range of 13.8 to 14.4 Gyr for NGC 6397, 14.75 Gyr within the range of 14.50 to 15.40 Gyr for M92, and 16.0 Gyr within the range of 15.9 to 16.3 Gyr for M3.

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Stellar Populations in NGC 1399 Traced by Globular Clusters from a Wide-Field Study,. The cluster system contains . clusters and the specific frequency is found to be . in the V band. NGC 1399 shows a pronounced color gradient, which can be interpreted by field populations that are genuinely related to the red and the blue cluster populations.

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Conference proceedings 2003chapter, followed by a chapter on young star clusters. Then come four chapters reviewing the globular cluster system of early-type, late-type and dwarf galaxies, as well as of groups of galaxies. One chapter is dedicated to stellar population models and their applications to the field. Finally a cha

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只看該作者 · 發(fā)表于 2025-3-29 21:14:39

Uncovering the NGC 5128 Globular Cluster System, the nearest large E galaxy (.), provides an important link to studies of extragalactic GCSs. But its proximity, combined with a moderately low Galactic latitude ( .) and a longitude ( .) only . from the Galactic center, mean that the global properties of this important GCS have been difficult to determine.

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1431-2433 the first chapter, followed by a chapter on young star clusters. Then come four chapters reviewing the globular cluster system of early-type, late-type and dwarf galaxies, as well as of groups of galaxies. One chapter is dedicated to stellar population models and their applications to the field. Fin

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