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

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樓主: dilate
31#
發(fā)表于 2025-3-26 22:57:13 | 只看該作者
32#
發(fā)表于 2025-3-27 04:32:21 | 只看該作者
Globular Clusters, Galactic Nuclei and Supermassive Black Holesith those of the globular clusters. A similar comparison between the nuclei and the supermassive black holes found in many massive galaxies points to an unforseen causal relationship between these two types of ..
33#
發(fā)表于 2025-3-27 08:18:26 | 只看該作者
1431-2433 tary material: .The principal question of whether and how globular clusters can contribute to a better understanding of galaxy formation and evolution is perhaps the main driving force behind the overall endeavour of studying globular cluster systems. Naturally, this splits up into many individual p
34#
發(fā)表于 2025-3-27 11:56:03 | 只看該作者
35#
發(fā)表于 2025-3-27 14:38:36 | 只看該作者
36#
發(fā)表于 2025-3-27 18:08:16 | 只看該作者
Mathematics and Its Applicationsse data holdings also have enormous potential for educational purposes from pre-college through non-majors courses and expert course curricula in universities. This paper focuses on software services and tools of use to researchers and will concentrate especially on opportunities presented by the National Virtual Observatory.
37#
發(fā)表于 2025-3-27 22:39:21 | 只看該作者
38#
發(fā)表于 2025-3-28 04:17:38 | 只看該作者
39#
發(fā)表于 2025-3-28 09:50:52 | 只看該作者
Sectionally Complemented Latticeshrough hydrogen-burning at high temperatures and then lost by more massive and faster evolving stars (and perhaps mixed with some original gas). Within this framework we present a new method to derive the Initial Mass Function of the polluter stars.
40#
發(fā)表于 2025-3-28 11:18:25 | 只看該作者
Abundance Anomalies in Galactic Globular Clusters – Looking for the Stellar Culpritshrough hydrogen-burning at high temperatures and then lost by more massive and faster evolving stars (and perhaps mixed with some original gas). Within this framework we present a new method to derive the Initial Mass Function of the polluter stars.
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