Collisional excitation of interstellar cyclopropenylidene.
Theoretical rotational excitation rates were computed for C3H2 in collisions with He atoms at temperatures from 30 to 120 K.  The intermolecular forces were obtained from accurate self-consistent field and perturbation theory calculations, and collision dynamics were treated within the infinite-order sudden approximation.  The accuracy of the latter was examined by comparing with the more exact coupled states approximation.
Green
S
S
NASA/Goddard Space Flight Center, Institute for Space Studies, New York, USA.
DeFrees
D J
DJ
McLean
A D
AD
D055580:Astronomical Phenomena; D001256:Astronomy; D019471:Elementary Particle Interactions; D005118:Extraterrestrial Environment; D006371:Helium / Q000032:analysis / Q000737:chemistry*; D006844:Hydrocarbons, Cyclic / Q000032:analysis / Q000737:chemistry*; D008958:Models, Molecular; D016082:Solar System; D013696:Temperature
D006844:Hydrocarbons, Cyclic; D006371:Helium