Primordial binaries and globular cluster evolution

Details Primordial binaries and globular cluster evolution Primordial binaries and globular cluster evolution

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989natur.339...40g&link_type=abstract

Nature (ISSN 0028-0836), vol. 339, May 4, 1989, p. 40-42.

Astronomy and Astrophysics

Astronomy

93

Astronomical Models, Binary Stars, Globular Clusters, Cosmology, Galactic Evolution, Giant Stars

Scientific paper

The most conservative solution to the problem of the energy source of globular clusters reexpanding after core collapse is explored. It is suggested that primordial binaries could provide the necessary energy, and it is shown that this mechanism leads to relatively large core sizes containing about one percent of the total cluster mass. Such a cluster would have a resolvable core consisting mostly of binaries.

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