Sesana, Alberto Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;
APJ_719_1_851.pdf (beliebiger Volltext), 2MB
Sesana, A. (2010). Self Consistent Model for the Evolution of Eccentric Massive Black Hole Binaries in Stellar Environments: Implications for Gravitational Wave Observations. Astrophysical Journal, 719: 851. doi:10.1088/0004-637X/719/1/851.