The Globular Cluster Mass Function as a Remnant of Violent Birth

Details The Globular Cluster Mass Function as a Remnant of Violent Birth The Globular Cluster Mass Function as a Remnant of Violent Birth

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21631606e&link_type=abstract

American Astronomical Society, AAS Meeting #216, #316.06; Bulletin of the American Astronomical Society, Vol. 41, p.897

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Scientific paper

The log-normal shape of the mass function for metal-poor halo globular clusters is proposed to result from an initial M-2 power law modified rapidly by evaporation, collisions with clouds, and mutual cluster interactions in the dense environment of a redshift z 5-15 disk galaxy. Galaxy interactions subsequently spray these clusters into the galaxy group environment, where they fall into other growing galaxies and populate their halos. Clusters forming later in z 2-5 galaxies, and those formed during major mergers, produce metal-rich globulars. Monte Carlo models of evolving cluster populations demonstrate the early formation of a log-normal mass function for typical conditions in high-redshift galaxies.

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