Improved collisional excitation rates for interstellar water.
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 changed significantly.  Successive improvements to the theoretical description of this system now appear to have converged.
Green
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NASA Goddard Space Flight Center, Institute for Space Studies, New York 10025.
Maluendes
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McLean
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D055580:Astronomical Phenomena; D001256:Astronomy; D055598:Chemical Phenomena; D015392:Chemistry, Inorganic; D005118:Extraterrestrial Environment; D006371:Helium; D008872:Microwaves; D008956:Models, Chemical; D008958:Models, Molecular; D016082:Solar System; D013696:Temperature; D014867:Water / Q000737:chemistry*
D014867:Water; D006371:Helium