Green and Thaddeus 1974
Green, S., and P. Thaddeus, 1974: Rotational excitation of HCN by collisions. Astrophys. J., 191, 653-658.
Rate constants for rotational excitation of HCN by collisions with low-energy He atoms (kinetic temperature below 100°K) have been computed from first principles. The accuracy of individual rates is conservatively estimated to be ±50 percent above 30°K and within a factor of 2 below 20°K. These rates are also believed to be representative of excitation by collisions with H2.
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Green, S., and Thaddeus, P.: Rotational excitation of HCN by collisions, Astrophys. J., 191, 653-658, 1974.
Green, S., and P. Thaddeus (1974), Rotational excitation of HCN by collisions, Astrophys. J., 191, 653-658.
Green, S., and P. Thaddeus, 1974: Rotational excitation of HCN by collisions. Astrophys. J., 191, 653-658.
Green, S., & Thaddeus, P. 1974, Astrophys. J., 191, 653.
Green S, Thaddeus P. Rotational excitation of HCN by collisions, Astrophys J 1974;191:653-658.
S. Green, P. Thaddeus, Astrophys. J. 191, 653-658 (1974).
