NLTE H2 Cooling Function and Protogalactic Evolution
暂无分享,去创建一个
[1] J. Shull,et al. Molecular processes and gravitational collapse in intergalactic shocks , 1986 .
[2] P. Shapiro,et al. Hydrogen Molecules and the Radiative Cooling of Pregalactic Shocks II: Low Velocity Shocks at High Redshift , 1985 .
[3] J. Smith. Cloud-cloud collisions in the interstellar medium , 1980 .
[4] D. Hollenbach,et al. Molecule formation and infrared emission in fast interstellar shocks. I Physical processes , 1979 .
[5] J. Hutchins. The thermal effects of H 2 molecules in rotating and collapsing spheroidal gas clouds. , 1976 .
[6] W. Saslaw,et al. Molecular Hydrogen in Pre-galactic Gas Clouds , 1967, Nature.
[7] M. Mcdowell. On the formation of H2 in H I regions , 1961 .
[8] A. Dalgarno,et al. The Quadrupole Vibration-Rotation Transition Probabilities of Molecular Hydrogen , 1977 .