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Consequences of Dynamical Disruption and Mass Segregation for the Binary Frequencies of Star Clusters
Aaron M. Geller, Richard de Grijs, Chengyuan Li +1
The massive (13,000-26,000 Msolar), young (15-30 Myr) Large Magellanic Cloud star cluster NGC 1818 reveals an unexpected increasing binary frequency with radius for F-type stars (1…
Comparing the White Dwarf Cooling Sequences in 47 Tuc and NGC 6397
Harvey B. Richer, Ryan Goldsbury, Jeremy Heyl +7
Using deep Hubble Space Telescope imaging, color-magnitude diagrams are constructed for the globular clusters 47 Tuc and NGC 6397. As expected, because of its lower metal abundance…
Stars on the run: escaping from stellar clusters
G. R. I. Moyano Loyola, J. R. Hurley
A significant proportion of Milky Way stars are born in stellar clusters, which dissolve over time so that the members become part of the disc and halo populations of the Galaxy. I…
The Influence of Orbital Eccentricity on Tidal Radii of Star Clusters
Jeremy J. Webb, William E. Harris, Alison Sills +1
We have performed N-body simulations of star clusters orbiting in a spherically symmetric smooth galactic potential. The model clusters cover a range of initial half-mass radii and…