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Neutron Star and Black Hole Binaries in Dense Star Clusters (P7)

Neutron Star and Black Hole Binaries in Dense Star Clusters (P7)

Neutron Star and Black Hole Binaries in Dense Star Clusters

Neutron Star and Black Hole Binaries in Dense Star Clusters (P7) Hyung Mok Lee (Seoul National Univ.) Dense star clusters can host neuron stars and black holes These stars can form binaries via 3-body interactions Hardening occurs as a result of encounters Eventually binaries get kicked out since the recoil energy binding E. Some fraction of the ejected binaries go into merger in Hubble time Rate is estimated to be ~10 -6 yr -1 Giant ellipticals have more star clusters/mass good place to look for them Red: Maximum hardness before ejection Shallow potential (i.e., globular clusters) Deep potential (i.e., galactic nuclei

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