Physical Interactions between Stars
暂无分享,去创建一个
[1] P. Hut. Hard binary-single star scattering cross sections for equal masses , 1984 .
[2] J. Goodman. Homologous evolution of stellar systems after core collapse , 1984 .
[3] S. Djorgovski,et al. Surface photometry in cores of globular clusters , 1984 .
[4] J. Krolik. Main-sequence binaries, contact binaries, and blue stragglers in globular clusters , 1983, Nature.
[5] S. Mikkola. Encounters of binaries – I. Equal energies , 1983 .
[6] H. Cohn,et al. Late core collapse in star clusters and the gravothermal instability , 1980 .
[7] R. Mathieu,et al. Random gravitational encounters and the evolution of spherical systems. VIII. Clusters with an initial distribution of binaries , 1980 .
[8] P. P. Eggleton,et al. On the consequences of the gravothermal catastrophe , 1980 .
[9] S. Shapiro,et al. Two-body tidal dissipation in large N-body systems , 1978 .
[10] S. M. Fall,et al. An approximate theory for the core collapse of two-component gravitating systems , 1978 .
[11] C. Pritchet. Near-infrared velocity dispersions for the nuclear bulges of M31 and M81 , 1978 .
[12] W. H. Press,et al. On formation of close binaries by two-body tidal capture , 1977 .
[13] Martin J. Rees,et al. Tidal capture formation of binary systems and X-ray sources in globular clusters. , 1975 .