Dynamical Formation of Compact Object Binaries in Globular Clusters

Details Dynamical Formation of Compact Object Binaries in Globular Clusters Dynamical Formation of Compact Object Binaries in Globular Clusters

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008head...10.2401f&link_type=abstract

American Astronomical Society, HEAD meeting #10, #24.01

Astronomy and Astrophysics

Astronomy

Scientific paper

Although dense stellar systems such as globular clusters have long been known to be overabundant per unit mass in X-ray binaries, it is only recently that theory and observations have begun to converge on a basic understanding of the formation and evolution of such systems in dense stellar environments. I will discuss what we have learned about their formation, and describe what observations of their populations have taught us about the properties of the clusters in which they reside.

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