Bieniek and Green 1983
Bieniek, R.J., and S. Green, 1983: Collisional rates for vibrational-rotational transitions in circumstellar SiO masers. Astrophys. J., 265, L29-L33, doi:10.1086/183952.
Calculations for rotational population inversion in circumstellar SiO masers require collisional rates for vibrational-rotational transitions. This paper reports quantum mechanical, state-to-state collisional rate coefficients for pure rotational and vibrational-rotational transitions among the first three vibrational states of SiO. These are expressed in terms of simple two-parameter power-law fits accurate in the temperature range 1000-3000 K.
Citation Styles
Show: ACP, AGU, AMS, ApJ, JQSRT, Science style
Bieniek, R.J., and Green, S.: Collisional rates for vibrational-rotational transitions in circumstellar SiO masers, Astrophys. J., 265, L29-L33, doi:10.1086/183952, 1983.
Bieniek, R.J., and S. Green (1983), Collisional rates for vibrational-rotational transitions in circumstellar SiO masers, Astrophys. J., 265, L29-L33, doi:10.1086/183952.
Bieniek, R.J., and S. Green, 1983: Collisional rates for vibrational-rotational transitions in circumstellar SiO masers. Astrophys. J., 265, L29-L33, doi:10.1086/183952.
Bieniek, R.J., & Green, S. 1983, Astrophys. J., 265, L29, doi:10.1086/183952.
Bieniek RJ, Green S. Collisional rates for vibrational-rotational transitions in circumstellar SiO masers, Astrophys J 1983;265:L29-L33. doi:10.1086/183952.
R.J. Bieniek, S. Green, Astrophys. J. 265, L29-L33, doi:10.1086/183952 (1983).
