Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..222..210r&link_type=abstract
In: After the first three minutes; Proceedings of the 1st Astrophysics Workshop, Univ. of Maryland, College Park, Oct. 15-17, 19
Astronomy and Astrophysics
Astrophysics
Cosmology, Galactic Evolution, Globular Clusters, Universe, Baryons, Density Distribution, Galactic Mass, Gravitational Collapse
Scientific paper
The idea of pregalactic formation of globular clusters is tested by assuming that all primordial fluctuations above a fixed threshold sigma defined globally over the whole universe survive as globulars. For a density threshold level of roughly 2.8 sigma, adequate fits are achieved to cluster radii and densities, the mass fraction of globular versus Hubble type, the radial density profile of globulars within galaxies, and the globular luminosity function.
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