Green et al. 1993
Green, S., S. Maluendes, and A.D. McLean, 1993: Improved collisional excitation rates for interstellar water. Astrophys. J. Supp. Series, 85, 181-185, doi:10.1086/191760.
Theoretical rate constants among the lowest 45 para and 45 ortho rotational levels of water in collisions with He atoms have been calculated for temperatures between 20 and 2000 K using a recently improved theoretical interaction potential. These values are about 30-40% larger than those reported previously (Palma et al. 1988b) but relative sizes of different state-to-state rates have not been changed significantly. Successive improvements to the theoretical description of this system now appear to have converged.
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Green, S., Maluendes, S., and McLean, A.D.: Improved collisional excitation rates for interstellar water, Astrophys. J. Supp. Series, 85, 181-185, doi:10.1086/191760, 1993.
Green, S., S. Maluendes, and A.D. McLean (1993), Improved collisional excitation rates for interstellar water, Astrophys. J. Supp. Series, 85, 181-185, doi:10.1086/191760.
Green, S., S. Maluendes, and A.D. McLean, 1993: Improved collisional excitation rates for interstellar water. Astrophys. J. Supp. Series, 85, 181-185, doi:10.1086/191760.
Green, S., Maluendes, S., & McLean, A.D. 1993, Astrophys. J. Supp. Series, 85, 181, doi:10.1086/191760.
Green S, Maluendes S, McLean AD. Improved collisional excitation rates for interstellar water, Astrophys J Supp Series 1993;85:181-185. doi:10.1086/191760.
S. Green, S. Maluendes, A.D. McLean, Astrophys. J. Supp. Series 85, 181-185, doi:10.1086/191760 (1993).
