1
Introduction
1.1
Overview of BH-NS binaries
1.2
Tidal problem around a BH: Effects of BH spin and the NS EOS
1.3
Why is the merger of BH-NS binaries important?
1.4
General relativistic study of BH-NS binaries in quasi-equilibrium states
1.5
Non-relativistic simulation for the merger
1.6
Stable mass transfer occurs or not
1.7
General relativistic study of late inspiral and merger
1.8
Outline and notation
Living Rev. Relativity
14, (2011), 6
http://www.livingreviews.org/lrr-2011-6
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