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- W2020129960 abstract "Abstract Evidence favouring a Gaussian initial mass function for systems of old globular clusters has accumulated over recent years. We show that a bell-shaped mass function may be the imprint of expulsion from protoclusters of the leftover star forming gas due to supernova activity. Owing to the corresponding weakening of its gravitational potential, a protocluster retains a fraction only of its newly formed stars. The mass fraction of bound stars extends from zero to unity depending on the star formation efficiency achieved by the protoglobular cloud. We investigate how such wide variations affect the mapping of the protoglobular cloud mass function to the initial globular cluster mass function. We conclusively demonstrate that the universality of the globular cluster mass function originates from a common protoglobular cloud mass-scale of about 10 6 M ⊙ among galaxies. Moreover, gas removal during star formation in massive gas clouds is highlighted as the likely prime cause of the predominance of field stars in the Galactic Halo." @default.
- W2020129960 created "2016-06-24" @default.
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- W2020129960 date "2007-09-01" @default.
- W2020129960 modified "2023-09-23" @default.
- W2020129960 title "The Origin of the Universal Globular Cluster Mass Function" @default.
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- W2020129960 doi "https://doi.org/10.1017/s1743921308016062" @default.
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