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

聰明

https://doi.org/10.1007/978-3-540-76961-3Accretion; Galaxy; Galaxy Evolution; Galaxy Formation; Globular Clusters; Star Clusters

MAPLE

Tom Richtler,S?ren LarsenComprehensive coverage of the field of Globular Cluster astrophysics and its relevance for galaxy formation and evolution.Includes supplementary material:

背叛者

Amplify

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

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.

誘騙

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

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.

污點(diǎn)

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.

無(wú)王時(shí)期,

Nonthreatening