Are Globular Clusters the Remnant Nuclei of Progenitor Disk Galaxies?

Torsten Boeker

doi:10.1086/527033

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arXiv · 0711.4542

Are Globular Clusters the Remnant Nuclei of Progenitor Disk Galaxies?

Torsten Boeker

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Abstract

The globular cluster system of a typical spheroidal galaxy makes up about 0.25% of the total galaxy mass (McLaughlin 1999). This is roughly the same mass fraction as contained in the nuclear star clus- ter (or stellar nucleus) present in most nearby low-mass galaxies. Motivated by this "coincidence", this Letter discusses a scenario in which globular clusters of present-day galaxies are the surviving nuclei of the dwarf galaxies that - according to the hierarchical merging paradigm of galaxy forma- tion - constitute the "building blocks" of present-day massive galaxies. This scenario, which was first suggested by Freeman (1993), has become more attractive recently in the light of studies that demonstrate a complex star formation history in a number of massive globular clusters.

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Torsten Boeker. 2007-11-28. Are Globular Clusters the Remnant Nuclei of Progenitor Disk Galaxies?. https://doi.org/10.1086/527033

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