聪明
发表于 2025-3-25 06:20:42
https://doi.org/10.1007/978-3-540-76961-3Accretion; Galaxy; Galaxy Evolution; Galaxy Formation; Globular Clusters; Star Clusters
MAPLE
发表于 2025-3-25 07:46:09
Tom Richtler,Søren LarsenComprehensive coverage of the field of Globular Cluster astrophysics and its relevance for galaxy formation and evolution.Includes supplementary material:
背叛者
发表于 2025-3-25 15:38:33
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Amplify
发表于 2025-3-25 16:16:40
Partially Ordered Sets and Lattices,lium abundance (Fig. 2). The presence of super-helium-rich populations in some globular clusters suggests that a third parameter, other than metallicity and age, also influences the CMD morphology of these clusters.
Nonflammable
发表于 2025-3-25 21:31:57
Sydney Bulman-Fleming,Kenneth McDowellstellar populations, such as GCs and elliptical galaxies. The new isochrones and HB tracks well reproduce the observed color magnitude diagrams of Galactic GCs, including peculiar features observed in the HB and MS of ω Centauri and NGC 2808.
诱骗
发表于 2025-3-26 02:24:59
Super-He-Rich Populations in Globular Clusterslium abundance (Fig. 2). The presence of super-helium-rich populations in some globular clusters suggests that a third parameter, other than metallicity and age, also influences the CMD morphology of these clusters.
Analogy
发表于 2025-3-26 07:01:13
New Yonsei-Yale (, ,) Isochrones and Horizontal-Branch Evolutionary Tracks with Helium Enhancementsstellar populations, such as GCs and elliptical galaxies. The new isochrones and HB tracks well reproduce the observed color magnitude diagrams of Galactic GCs, including peculiar features observed in the HB and MS of ω Centauri and NGC 2808.
污点
发表于 2025-3-26 11:33:34
Open Questions in the Globular Cluster – Galaxy Connectionves today. In turn, I then look at todays pending problems on individual star clusters (e.g. measuring their integrated properties), on globular cluster systems, and finally on the link to galaxy formation and evolution. I end up being not very conclusive.
无王时期,
发表于 2025-3-26 14:51:48
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Nonthreatening
发表于 2025-3-26 19:41:43
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